Tuesday, November 29, 2022

In Memoriam: Celebrities Lost 1680



Denzil Holles, 1st Baron Holles

Jan Swammerdam

Catherine Majvoisin

Rene Le Bossu

Francois VI, duc de la Rochefouchuld

Nicolas Fouquet

Shivaji Bhonsle (Chhatrapati Shivaji Mahara)

Kateri Tekakwitha (Lily of the Mohawks)

Abraham Meyerle

Joachim Neander

Johan  Goranson Gyllenstierna

Louis Moreri

John Wilmot, 2nd Earl of Rochester

Thomas Butler, Earl of Ossory

Jean Eudes

William Bedloe

Johann Georg II, Elector of Saxony

Ferdinand Bulb

Thomas Blood

Joan Cererols

Per Brahe

Henry Marten

Baldassare Ferri

Marco Uccellini

Emperor Go-Mizunoo, 108th Emperor of Japan

 

Happy Birthday: November 29, 2022

 



Howie Mandel, 67

Anna Faris, 46

John Mayall, 89

Diane Ladd, 87

Chuck Mangione, 82

Felix Cavaliere, 80

Jeff Fahey, 70

Joel Coen, 68

Cathy Moriarty, 62

Kim Delaney, 61

Tom Sizemore, 61

Andrew McCarthy, 60

Neill Barry, 57

Jonathan Knight, 54

Larry Joe Campbell, 52

Frank Delgado, 52

Paola Turbay, 52

Crowder, 51

Gena Lee Nolin, 51

Brian Baumgartner, 50

Julian Ovenden, 47

James Fortune, 45

Lauren German, 44

The Game, 43

Ringo Garza, 41

John Milhiser, 41

Lucas Black, 40

Diego Boneta, 32

Lovie Simone, 24

Jerry "The King" Lawer, 73

Christian Doppler (November 29, 1803-March 17, 1853)

Louisa May Alcott (November 29, 1832-March 6, 1888)

C. S. Lewis (November 29, 1898-Novmeber 22, 1963)

Gary Shandling (November 29, 1949-March 24, 2016)

In Memoriam: Celebrities Lost 1681



Richard Allestree

Francesco Nigetti

Frans van Mieri the Elder

Alfonso Marsh

Pedro Calderon de la Barca

William Lilly

Oliver Plunkett, Catholic Archbishop

Fjodor Aleksejevitsj, Tsar of Russia

Georg Neumark

Urian Oakes

Nikon (Nikita Minin)

Nicolaas Heinsius

Gerard Terborch the Younger

Richard Alleine

 

Happy Birthday: November 28, 2022

 



Berry Gordy, 93

Randy  Newman, 79

Paul Shaffer, 73

Ed Harris, 72

Alfonso Cuaron, 61

Jon Stewart, 60

Mary Elizabeth Winstead, 38

Karen Gillan, 35

Bruce Channel, 82

S. Epatha Merkerson, 70

Kristine Arnold, 66

Judd Nelson, 63

Matt Cameron, 60

Jane Sibbett, 60

Garcelle Beauvais, 56

Dawn Robinson, 54

Gina Tognoni, 49

apl. de. ap., 48

Malcolm Goodwin, 47

Ryan Kwanten, 46

Aimee Garcia, 46

Chamillionaire, 43

Daniel Henney, 43

Rostam Batmanglij, 39

Tyler Glenn, 39

Trey Songz, 38

Scarlett Pomers, 34

Bryshere, 29

Paul Warfield, 80

William Blake (November 28, 1757-August 12, 1827)

Henry Bacon (November 28, 1866-February 16, 1924)

Anna Nicole Smith (November 28, 1967-February 8, 2007)

In Memoriam: Celebrities Lost 1682



Simon van Leeuwen

Abraham de Wicquefort

Alessandro Stradella

Jacob van Ruisdael

Franz Egan of Furstenberg, Bavarian Catholic Archbishop

Bartolome Esteban Murillo

Avvakum, Russian Orthodox Archpriest

Theodorus III, Tsar of Russia

Jean Picard

Johann Heinrich Kittel

Juan Cuaramuel y Lobkowitz

John Ferrabosco

Thomas Browne

Claudie Lorruin

Prince Rupert of the Rhine

 

Happy Birthday: November 27, 2022



Kathryn Bigelow, 71

Bill Nye, 67

Fisher Stevens, 59

Robin Givens, 58

Jaleel White, 46

Alison Pill, 37

William Fichtner, 66

Charlie Burchill, 63

Michael Rispoli, 62

Charlie Benante, 60

Mike Bordin, 60

Michael Vartan, 54

Elizabeth Marvel, 53

Skoob, 51

Kirk Acevedo, 51

Twista, 50

Lashanda Lynch, 35

Caroline Kennedy, 65

Robert Livingston (November 27, 1746-February 26, 1813)

"Buffalo" Bob Smith (November 27, 1917-July 30, 1998)

Bruce Lee (November 27, 1940-July 20, 1973)

Jimi Hendrix (November 27, 1942-September 18, 1970)

 

Saturday, November 26, 2022

In Memoriam: Celebrities Lost 1683



Philip Warwick

Anthony Ashley Cooper, 1st Earl of Shaftesbury

Nicolaes Pietersz Berchem

Thomas Killigrew

Yaoya Oshichi

Stjepan  Gradic

Francois-Eudes de Mezeray

Arthur Capell, 1st Earl of Essex

Lord William Russell

Maria Theresa of Spain

Charles Hart

John Owen

Christoph Schultze

Jean-Baptiste Colbert

Algernon Sidney

Afonso VI, King of Portugal

Philipp Friedrich Boddecker

John Oldham

Izaak Walton

Kara Mustafa Pasha

 

Happy Birthday: November 26, 2022



Tina Turner, 83

John McVie, 77

Peter Facinelli, 49

DJ Khaled, 47

Rita Ora, 32

Rich Little, 84

Jean Terrell, 78

Marianne Muellerleile, 74

Scott Jacoby, 66

Jamie Rose, 63

Linda Davis, 60

Scott Adsit, 56

Tammy Lynn Michaels, 48

Maia Campbell, 46

Joe Nichols, 46

Randy Armstrong, 44

Anthony Armstrong, 44

Jessica Bowman, 42

Natasha Bedingfield, 41

Jessica Camacho, 40

Mike Gossin, 38

Ben Wysocki, 38

Lil Fizz, 37

Aubrey Collins, 35

Aubrey Peeples, 29

John Harvard (November 26?, 1607-September 14, 1638)

Willis Carrier (November 26, 1876-October 7, 1950)

Charles M. Schultz (November 26, 1922-February 12, 2000)

Robert Goulet (November 26, 1933-October 30, 2007)

 

In Memoriam: Celebrities Lost 1684



Claude Audran II


Caspar Netscher

Pietro Andrea Ciani

Pieter van den Abeelen

William Brouncker

Gonzales Coques

Roger Williams

John Nevison

Henri Dumont

Edme Mariotte

Adriaen Backer

John Rogers

Peter Gunning

Elena Covinaro Piscopia

George Booth, 1st Baron Delamer

John Uytenhace van Lacks

Johannes Antonides van der Goes

Pierrie Corneille

 

Happy Birthday: November 25, 2022



Ben Stein, 78

John Larroquette, 75

Amy Grant, 62

Billy Burke, 56

Jill Hennessy 53

Christina Applegate, 51

Joey Chestnut, 39

Katie Cassidy, 36

Kathryn Crosby, 89

Bob Lind, 80

Bruno Tunioli, 67

Scott Mercado, 58

Tim Armstrong, 57

Steve Harris, 57

Stacy Lattisaw, 56

Rodney Sheppard, 56

Erick Sermon, 54

Eddie Steeples, 49

Kristian Nairn, 47

Jill Flint, 45

Jerry Ferrara, 43

Valerie Azlynn, 42

Stephanie Itsu, 32

Jamie Grace, 31

Bernie Kosar, 59

Barbara Pierce Bush, 41

Jenna Bush Hager, 41

Andrew Carnegie (November 25, 1835-August 11,1919)

Pope John XXII (November 25, 1249-December 4, 1334)

Joe DiMaggio (November 25, 1914-March 1999)

Ricardo Montalban (November 25, 1920-January 4, 2009)

John F. Kennedy, Jr. (November 25, 1960-July 16, 1999)

 

Thursday, November 24, 2022

Our Solar System: Comets Part II

 


Comets and impact on life


Many comets and asteroids collided with Earth in its early stages. Many scientists think that comets bombarding the young Earth about 4 billion years ago brought the vast quantities of water that now fill Earth's oceans, or at least a significant portion of it. Others have cast doubt on this idea. The detection of organic molecules, including poly-cyclic aromatic hydrocarbons, in significant quantities in comets has led to speculation that comets or meteorites may have brought the precursors of life—or even life itself—to Earth. In 2013 it was suggested that impacts between rocky and icy surfaces, such as comets, had the potential to create the amino acids that make up proteins through shock synthesis. The speed at which the comets entered the atmosphere, combined with the magnitude of energy created after initial contact, allowed smaller molecules to condense into the larger macro-molecules that served as the foundation for life. In 2015, scientists found significant amounts of molecular oxygen in the out-gassings of comet 67P, suggesting that the molecule may occur more often than had been thought, and thus less an indicator of life as has been supposed.


It is suspected that comet impacts have, over long timescales, also delivered significant quantities of water to Earth's Moon, some of which may have survived as lunar ice. Comet and meteoroid impacts are also thought to be responsible for the existence of tektites and australites.


Fear of comets


Fear of comets as acts of God and signs of impending doom was highest in Europe from AD 1200 to 1650. The year after the Great Comet of 1618, for example, Gotthard Arthusius published a pamphlet stating that it was a sign that the Day of Judgment was near. He listed ten pages of comet-related disasters, including "earthquakes, floods, changes in river courses, hail storms, hot and dry weather, poor harvests, epidemics, war and treason and high prices".


By 1700 most scholars concluded that such events occurred whether a comet was seen or not. Using Edmond Halley's records of comet sightings, however, William Whiston in 1711 wrote that the Great Comet of 1680 had a periodicity of 574 years and was responsible for the worldwide flood in the Book of Genesis, by pouring water on Earth. His announcement revived for another century fear of comets, now as direct threats to the world instead of signs of disasters. Spectroscopic analysis in 1910 found the toxic gas cyanogen in the tail of Halley's Comet, causing panicked buying of gas masks and quack "anti-comet pills" and "anti-comet umbrellas" by the public.


Fate of comets


If a comet is traveling fast enough, it may leave the Solar System. Such comets follow the open path of a hyperbola, and as such, they are called hyperbolic comets. Solar comets are only known to be ejected by interacting with another object in the Solar System, such as Jupiter. An example of this is Comet C/1980 E1, which was shifted from an orbit of 7.1 million years around the Sun, to a hyperbolic trajectory, after a 1980 close pass by the planet Jupiter. Interstellar comets such as 1I/ʻOumuamua and 2I/Borisov never orbited the Sun and therefore do not require a 3rd-body interaction to be ejected from the Solar System.


Volatiles exhausted


Jupiter-family comets and long-period comets appear to follow very different fading laws. The JFCs are active over a lifetime of about 10,000 years or ~1,000 orbits whereas long-period comets fade much faster. Only 10% of the long-period comets survive more than 50 passages to small perihelion and only 1% of them survive more than 2,000 passages. Eventually most of the volatile material contained in a comet nucleus evaporates, and the comet becomes a small, dark, inert lump of rock or rubble that can resemble an asteroid. Some asteroids in elliptical orbits are now identified as extinct comets. Roughly six percent of the near-Earth asteroids are thought to be extinct comet nuclei.


Breakup and collisions


The nucleus of some comets may be fragile, a conclusion supported by the observation of comets splitting apart. A significant cometary disruption was that of Comet Shoemaker–Levy 9, which was discovered in 1993. A close encounter in July 1992 had broken it into pieces, and over a period of six days in July 1994, these pieces fell into Jupiter's atmosphere—the first time astronomers had observed a collision between two objects in the Solar System. Other splitting comets include 3D/Biela in 1846 and 73P/Schwassmann–Wachmann from 1995 to 2006. Greek historian Ephorus reported that a comet split apart as far back as the winter of 372–373 BC. Comets are suspected of splitting due to thermal stress, internal gas pressure, or impact.


Comets 42P/Neujmin and 53P/Van Biesbroeck appear to be fragments of a parent comet. Numerical integrations have shown that both comets had a rather close approach to Jupiter in January 1850, and that, before 1850, the two orbits were nearly identical.


Some comets have been observed to break up during their perihelion passage, including great comets West and Ikeya–Seki. Biela's Comet was one significant example when it broke into two pieces during its passage through the perihelion in 1846. These two comets were seen separately in 1852, but never again afterward. Instead, spectacular meteor showers were seen in 1872 and 1885 when the comet should have been visible. A minor meteor shower, the Andromedids, occurs annually in November, and it is caused when Earth crosses the orbit of Biela's Comet.


Some comets meet a more spectacular end – either falling into the Sun or smashing into a planet or other body. Collisions between comets and planets or moons were common in the early Solar System: some of the many craters on the Moon, for example, may have been caused by comets. A recent collision of a comet with a planet occurred in July 1994 when Comet Shoemaker–Levy 9 broke up into pieces and collided with Jupiter.


The names given to comets have followed several different conventions over the past two centuries. Prior to the early 20th century, most comets were referred to by the year when they appeared, sometimes with additional adjectives for particularly bright comets; thus, the "Great Comet of 1680", the "Great Comet of 1882", and the "Great January Comet of 1910".


After Edmond Halley demonstrated that the comets of 1531, 1607, and 1682 were the same body and successfully predicted its return in 1759 by calculating its orbit, that comet became known as Halley's Comet. Similarly, the second and third known periodic comets, Encke's Comet and Biela's Comet, were named after the astronomers who calculated their orbits rather than their original discoverers. Later, periodic comets were usually named after their discoverers, but comets that had appeared only once continued to be referred to by the year of their appearance.


In the early 20th century, the convention of naming comets after their discoverers became common, and this remains so today. A comet can be named after its discoverers or an instrument or program that helped to find it. For example, in 2019, astronomer Gennadiy Borisov observed a comet that appeared to have originated outside of the solar system; the comet was named 2I/Borisov after him.


History of study


From ancient sources, such as Chinese oracle bones, it is known that comets have been noticed by humans for millennia. Until the sixteenth century, comets were usually considered bad omens of deaths of kings or noble men, or coming catastrophes, or even interpreted as attacks by heavenly beings against terrestrial inhabitants.


Aristotle (384–322 BC) was the first known scientist to use various theories and observational facts to employ a consistent, structured cosmological theory of comets. He believed that comets were atmospheric phenomena, due to the fact that they could appear outside of the zodiac and vary in brightness over the course of a few days. Aristotle's cometary theory arose from his observations and cosmological theory that everything in the cosmos is arranged in a distinct configuration. Part of this configuration was a clear separation between the celestial and terrestrial, believing comets to be strictly associated with the latter. According to Aristotle, comets must be within the sphere of the moon and clearly separated from the heavens. Also in the 4th century BC, Apollonius of Myndus supported the idea that comets moved like the planets. Aristotelian theory on comets continued to be widely accepted throughout the Middle Ages, despite several discoveries from various individuals challenging aspects of it.


In the 1st century AD, Seneca the Younger questioned Aristotle's logic concerning comets. Because of their regular movement and imperviousness to wind, they cannot be atmospheric, and are more permanent than suggested by their brief flashes across the sky. He pointed out that only the tails are transparent and thus cloud-like, and argued that there is no reason to confine their orbits to the zodiac. In criticizing Apollonius of Myndus, Seneca argues, "A comet cuts through the upper regions of the universe and then finally becomes visible when it reaches the lowest point of its orbit." While Seneca did not author a substantial theory of his own, his arguments would spark much debate among Aristotle's critics in the 16th and 17th centuries.


Also in the 1st century, Pliny the Elder believed that comets were connected with political unrest and death. Pliny observed comets as "human like", often describing their tails with "long hair" or "long beard". His system for classifying comets according to their color and shape was used for centuries.


In India, by the 6th century astronomers believed that comets were celestial bodies that re-appeared periodically. This was the view expressed in the 6th century by the astronomers Varāhamihira and Bhadrabahu, and the 10th-century astronomer Bhaṭṭotpala listed the names and estimated periods of certain comets, but it is not known how these figures were calculated or how accurate they were. In 1301, the Italian painter Giotto was the first person to accurately and anatomically portray a comet. In his work Adoration of the Magi, Giotto's depiction of Halley's Comet in the place of the Star of Bethlehem would go unmatched in accuracy until the 19th century and be bested only with the invention of photography.


Astrological interpretations of comets proceeded to take precedence clear into the 15th century, despite the presence of modern scientific astronomy beginning to take root. Comets continued to forewarn of disaster, as seen in the Luzerner Schilling chronicles and in the warnings of Pope Callixtus III. In 1578, German Lutheran bishop Andreas Celichius defined comets as "the thick smoke of human sins... kindled by the hot and fiery anger of the Supreme Heavenly Judge". The next year, Andreas Dudith stated that "If comets were caused by the sins of mortals, they would never be absent from the sky."


Scientific approach


Crude attempts at a parallax measurement of Halley's Comet were made in 1456, but were erroneous. Regiomontanus was the first to attempt to calculate diurnal parallax by observing the great comet of 1472. His predictions were not very accurate, but they were conducted in the hopes of estimating the distance of a comet from the Earth.


In the 16th century, Tycho Brahe and Michael Maestlin demonstrated that comets must exist outside of Earth's atmosphere by measuring the parallax of the Great Comet of 1577. Within the precision of the measurements, this implied the comet must be at least four times more distant than from Earth to the Moon. Based on observations in 1664, Giovanni Borelli recorded the longitudes and latitudes of comets that he observed, and suggested that cometary orbits may be parabolic. Galileo Galilei, one of the most renowned astronomers to date, even attempted writings on comets in The Assayer. He rejected Brahe's theories on the parallax of comets and claimed that they may be a mere optical illusion. Intrigued as early scientists were about the nature of comets, Galileo could not help but throw about his own theories despite little personal observation. Maestlin's student Johannes Kepler responded to these unjust criticisms in his work Hyperaspistes. Jakob Bernoulli published another attempt to explain comets (Conamen Novi Systematis Cometarum) in 1682.


Also occurring in the early modern period was the study of comets and their astrological significance in medical disciplines. Many healers of this time considered medicine and astronomy to be inter-disciplinary and employed their knowledge of comets and other astrological signs for diagnosing and treating patients.


Isaac Newton, in his Principia Mathematica of 1687, proved that an object moving under the influence of gravity by an inverse square law must trace out an orbit shaped like one of the conic sections, and he demonstrated how to fit a comet's path through the sky to a parabolic orbit, using the comet of 1680 as an example. He describes comets as compact and durable solid bodies moving in oblique orbit and their tails as thin streams of vapor emitted by their nuclei, ignited or heated by the Sun. He suspected that comets were the origin of the life-supporting component of air. He also pointed out that comets usually appear near the Sun, and therefore most likely orbit it. On their luminosity, he stated, "The comets shine by the Sun's light, which they reflect," with their tails illuminated by "the Sun's light reflected by a smoke arising from [the coma]".


In 1705, Edmond Halley (1656–1742) applied Newton's method to 23 cometary apparitions that had occurred between 1337 and 1698. He noted that three of these, the comets of 1531, 1607, and 1682, had very similar orbital elements, and he was further able to account for the slight differences in their orbits in terms of gravitational perturbation caused by Jupiter and Saturn. Confident that these three apparitions had been three appearances of the same comet, he predicted that it would appear again in 1758–9. Halley's predicted return date was later refined by a team of three French mathematicians: Alexis Clairaut, Joseph Lalande, and Nicole-Reine Lepaute, who predicted the date of the comet's 1759 perihelion to within one month's accuracy. When the comet returned as predicted, it became known as Halley's Comet.


From his huge vaporing train perhaps to shake

Reviving moisture on the numerous orbs,

Thro' which his long ellipsis winds; perhaps

To lend new fuel to declining suns,

To light up worlds, and feed th' ethereal fire.


James Thomson The Seasons (1730; 1748)


As early as the 18th century, some scientists had made correct hypotheses as to comets' physical composition. In 1755, Immanuel Kant hypothesized in his Universal Natural History that comets were condensed from "primitive matter" beyond the known planets, which is "feebly moved" by gravity, then orbit at arbitrary inclinations, and are partially vaporized by the Sun's heat as they near perihelion. In 1836, the German mathematician Friedrich Wilhelm Bessel, after observing streams of vapor during the appearance of Halley's Comet in 1835, proposed that the jet forces of evaporating material could be great enough to significantly alter a comet's orbit, and he argued that the non-gravitational movements of Encke's Comet resulted from this phenomenon.


In the 19th century, the Astronomical Observatory of Padova was an epicenter in the observational study of comets. Led by Giovanni Santini (1787–1877) and followed by Giuseppe Lorenzoni (1843–1914), this observatory was devoted to classical astronomy, mainly to the new comets and planets orbit calculation, with the goal of compiling a catalog of almost ten thousand stars. Situated in the Northern portion of Italy, observations from this observatory were key in establishing important geodetic, geographic, and astronomical calculations, such as the difference of longitude between Milan and Padua as well as Padua to Fiume. In addition to these geographic observations, correspondence within the observatory, particularly between Santini and another astronomer Giuseppe Toaldo, about the importance of comet and planetary orbital observations.


In 1950, Fred Lawrence Whipple proposed that rather than being rocky objects containing some ice, comets were icy objects containing some dust and rock. This "dirty snowball" model soon became accepted and appeared to be supported by the observations of an armada of spacecraft (including the European Space Agency's Giotto probe and the Soviet Union's Vega 1 and Vega 2) that flew through the coma of Halley's Comet in 1986, photographed the nucleus, and observed jets of evaporating material.


On 22 January 2014, ESA scientists reported the detection, for the first definitive time, of water vapor on the dwarf planet Ceres, the largest object in the asteroid belt. The detection was made by using the far-infrared abilities of the Herschel Space Observatory. The finding is unexpected because comets, not asteroids, are typically considered to "sprout jets and plumes". According to one of the scientists, "The lines are becoming more and more blurred between comets and asteroids." On 11 August 2014, astronomers released studies, using the Atacama Large Millimeter/Submillimeter Array (ALMA) for the first time, that detailed the distribution of HCN, HNC, H2CO, and dust inside the comae of comets C/2012 F6 (Lemmon) and C/2012 S1 (ISON).


Spacecraft missions


The Halley Armada describes the collection of spacecraft missions that visited and/or made observations of Halley's Comet 1980s perihelion. The space shuttle Challenger was intended to do a study of Halley's Comet in 1986, but exploded shortly after being launched.


Deep Impact. Debate continues about how much ice is in a comet. In 2001, the Deep Space 1 spacecraft obtained high-resolution images of the surface of Comet Borrelly. It was found that the surface of comet Borrelly is hot and dry, with a temperature of between 26 to 71 °C (79 to 160 °F), and extremely dark, suggesting that the ice has been removed by solar heating and maturation, or is hidden by the soot-like material that covers Borrelly. In July 2005, the Deep Impact probe blasted a crater on Comet Tempel 1 to study its interior. The mission yielded results suggesting that the majority of a comet's water ice is below the surface and that these reservoirs feed the jets of vaporized water that form the coma of Tempel 1. Renamed EPOXI, it made a flyby of Comet Hartley 2 on 4 November 2010.


Ulysses. In 2007, the Ulysses probe unexpectedly passed through the tail of the comet C/2006 P1 (McNaught) which was discovered in 2006. Ulysses was launched in 1990 and the intended mission was for Ulysses to orbit around the sun for further study at all latitudes.


Stardust. Data from the Stardust mission show that materials retrieved from the tail of Wild 2 were crystalline and could only have been "born in fire", at extremely high temperatures of over 1,000 °C (1,830 °F). Although comets formed in the outer Solar System, radial mixing of material during the early formation of the Solar System is thought to have redistributed material throughout the proto-planetary disk. As a result, comets also contain crystalline grains that formed in the early, hot inner Solar System. This is seen in comet spectra as well as in sample return missions. More recent still, the materials retrieved demonstrate that the "comet dust resembles asteroid materials". These new results have forced scientists to rethink the nature of comets and their distinction from asteroids.


Rosetta. The Rosetta probe orbited Comet Churyumov–Gerasimenko. On 12 November 2014, its lander Philae successfully landed on the comet's surface, the first time a spacecraft has ever landed on such an object in history.


Classification


Approximately once a decade, a comet becomes bright enough to be noticed by a casual observer, leading such comets to be designated as great comets. Predicting whether a comet will become a great comet is notoriously difficult, as many factors may cause a comet's brightness to depart drastically from predictions. Broadly speaking, if a comet has a large and active nucleus, will pass close to the Sun, and is not obscured by the Sun as seen from Earth when at its brightest, it has a chance of becoming a great comet. However, Comet Kohoutek in 1973 fulfilled all the criteria and was expected to become spectacular but failed to do so. Comet West, which appeared three years later, had much lower expectations but became an extremely impressive comet.


The Great Comet of 1577 is a well-known example of a great comet. It passed near Earth as a non-periodic comet and was seen by many, including well-known astronomers Tycho Brahe and Taqi ad-Din. Observations of this comet led to several significant findings regarding cometary science, especially for Brahe.


The late 20th century saw a lengthy gap without the appearance of any great comets, followed by the arrival of two in quick succession—Comet Hyakutake in 1996, followed by Hale–Bopp, which reached maximum brightness in 1997 having been discovered two years earlier. The first great comet of the 21st century was C/2006 P1 (McNaught), which became visible to naked eye observers in January 2007. It was the brightest in over 40 years.


Sun-grazing comets


A sun-grazing comet is a comet that passes extremely close to the Sun at perihelion, generally within a few million kilometers. Although small sun-grazers can be completely evaporated during such a close approach to the Sun, larger sun-grazers can survive many perihelion passages. However, the strong tidal forces they experience often lead to their fragmentation.


About 90% of the sun-grazers observed with SOHO are members of the Kreutz group, which all originate from one giant comet that broke up into many smaller comets during its first passage through the inner Solar System. The remainder contains some sporadic sun-grazers, but four other related groups of comets have been identified among them: the Kracht, Kracht 2a, Marsden, and Meyer groups. The Marsden and Kracht groups both appear to be related to Comet 96P/Machholz, which is also the parent of two meteor streams, the Quadrantids and the Arietids.


Unusual comets


Of the thousands of known comets, some exhibit unusual properties. Comet Encke (2P/Encke) orbits from outside the asteroid belt to just inside the orbit of the planet Mercury whereas the Comet 29P/Schwassmann–Wachmann currently travels in a nearly circular orbit entirely between the orbits of Jupiter and Saturn. 2060 Chiron, whose unstable orbit is between Saturn and Uranus, was originally classified as an asteroid until a faint coma was noticed. Similarly, Comet Shoemaker–Levy 2 was originally designated asteroid 1990 UL3.


Largest


The largest known periodic comet is 95P/Chiron at 200 km in diameter that comes to perihelion every 50 years just inside of Saturn's orbit at 8 AU. The largest known Oort cloud comet is suspected of being Comet Bernardinelli-Bernstein at ≈150 km that will not come to perihelion until January 2031 just outside of Saturn's orbit at 11 AU. The Comet of 1729 is estimated to have been ≈100 km in diameter and came to perihelion inside of Jupiter's orbit at 4 AU.


Centaurs


Centaurs typically behave with characteristics of both asteroids and comets. Centaurs can be classified as comets such as 60558 Echeclus, and 166P/NEAT. 166P/NEAT was discovered while it exhibited a coma, and so is classified as a comet despite its orbit, and 60558 Echeclus was discovered without a coma but later became active, and was then classified as both a comet and an asteroid (174P/Echeclus). One plan for Cassini involved sending it to a centaur, but NASA decided to destroy it instead.


Observation


A comet may be discovered photographically using a wide-field telescope or visually with binoculars. However, even without access to optical equipment, it is still possible for the amateur astronomer to discover a sun-grazing comet online by downloading images accumulated by some satellite observatories such as SOHO. SOHO's 2000th comet was discovered by Polish amateur astronomer Michał Kusiak on 26 December 2010 and both discoverers of Hale–Bopp used amateur equipment (although Hale was not an amateur).


Lost


A number of periodic comets discovered in earlier decades or previous centuries are now lost comets. Their orbits were never known well enough to predict future appearances or the comets have disintegrated. However, occasionally a "new" comet is discovered, and calculation of its orbit shows it to be an old "lost" comet. An example is Comet 11P/Tempel–Swift–LINEAR, discovered in 1869 but unobservable after 1908 because of perturbations by Jupiter. It was not found again until accidentally rediscovered by LINEAR in 2001. There are at least 18 comets that fit this category.


In popular culture


The depiction of comets in popular culture is firmly rooted in the long Western tradition of seeing comets as harbingers of doom and as omens of world-altering change. Halley's Comet alone has caused a slew of sensationalist publications of all sorts at each of its reappearances. It was especially noted that the birth and death of some notable persons coincided with separate appearances of the comet, such as with writers Mark Twain (who correctly speculated that he'd "go out with the comet" in 1910) and Eudora Welty, to whose life Mary Chapin Carpenter dedicated the song "Halley Came to Jackson".


In times past, bright comets often inspired panic and hysteria in the general population, being thought of as bad omens. More recently, during the passage of Halley's Comet in 1910, Earth passed through the comet's tail, and erroneous newspaper reports inspired a fear that cyanogen in the tail might poison millions, whereas the appearance of Comet Hale–Bopp in 1997 triggered the mass suicide of the Heaven's Gate cult.


In science fiction, the impact of comets has been depicted as a threat overcome by technology and heroism (as in the 1998 films Deep Impact and Armageddon), or as a trigger of global apocalypse (Lucifer's Hammer, 1979) or zombies (Night of the Comet, 1984). In Jules Verne's Off on a Comet a group of people are stranded on a comet orbiting the Sun, while a large crewed space expedition visits Halley's Comet in Sir Arthur C. Clarke's novel 2061: Odyssey Three.


In Literature


The long-period comet first recorded by Pons in Florence on 15 July 1825 inspired Lydia Sigourney's humorous poem Wikisource-logo.svg The Comet of 1825. in which all the celestial bodies argue over the comet's appearance and purpose.


Footnotes


"I do not think that a comet is just a sudden fire, but that it is among the eternal works of nature." (Sagan & Druyan 1997, p. 26)


Seneca is quoted as stating, "Why ... are we surprised that comets, such a rare spectacle in the universe, are not yet grasped by fixed laws and that their beginning and end are not known, when their return is at vast intervals? ... The time will come when diligent research over very long periods of time will bring to light things which now lie hidden."



 

Our Solar System: Comets Part I




A comet is an icy, small Solar System body that, when passing close to the Sun, warms and begins to release gases, a process that is called out-gassing. This produces a visible atmosphere or coma, and sometimes also a tail. These phenomena are due to the effects of solar radiation and the solar wind acting upon the nucleus of the comet. Comet nuclei range from a few hundred meters to tens of kilometers across and are composed of loose collections of ice, dust, and small rocky particles. The coma may be up to 15 times Earth's diameter, while the tail may stretch beyond one astronomical unit. If sufficiently bright, a comet may be seen from Earth without the aid of a telescope and may subtend an arc of 30° (60 Moons) across the sky. Comets have been observed and recorded since ancient times by many cultures and religions.


Comets usually have highly eccentric elliptical orbits, and they have a wide range of orbital periods, ranging from several years to potentially several millions of years. Short-period comets originate in the Kuiper belt or its associated scattered disc, which lie beyond the orbit of Neptune. Long-period comets are thought to originate in the Oort cloud, a spherical cloud of icy bodies extending from outside the Kuiper belt to halfway to the nearest star. Long-period comets are set in motion towards the Sun from the Oort cloud by gravitational perturbations caused by passing stars and the galactic tide. Hyperbolic comets may pass once through the inner Solar System before being flung to interstellar space. The appearance of a comet is called an apparition.


Comets are distinguished from asteroids by the presence of an extended, gravitationally unbound atmosphere surrounding their central nucleus. This atmosphere has parts termed the coma (the central part immediately surrounding the nucleus) and the tail (a typically linear section consisting of dust or gas blown out from the coma by the Sun's light pressure or out-streaming solar wind plasma). However, extinct comets that have passed close to the Sun many times have lost nearly all of their volatile ices and dust and may come to resemble small asteroids. Asteroids are thought to have a different origin from comets, having formed inside the orbit of Jupiter rather than in the outer Solar System. The discovery of main-belt comets and active centaur minor planets has blurred the distinction between asteroids and comets. In the early 21st century, the discovery of some minor bodies with long-period comet orbits, but characteristics of inner solar system asteroids, were called Manx comets. They are still classified as comets, such as C/2014 S3 (PANSTARRS). Twenty-seven Manx comets were found from 2013 to 2017.


As of November 2021 there are 4584 known comets. However, this represents a very small fraction of the total potential comet population, as the reservoir of comet-like bodies in the outer Solar System (in the Oort cloud) is about one trillion. Roughly one comet per year is visible to the naked eye, though many of those are faint and unspectacular. Particularly bright examples are called "great comets". Comets have been visited by unmanned probes such as the European Space Agency's Rosetta, which became the first to land a robotic spacecraft on a comet, and NASA's Deep Impact, which blasted a crater on Comet Tempel 1 to study its interior.


Etymology


The word comet derives from the Old English cometa from the Latin comēta or comētēs. That, in turn, is a romanization of the Greek κομήτης 'wearing long hair', and the Oxford English Dictionary notes that the term (ἀστὴρ) κομήτης already meant 'long-haired star, comet' in Greek. Κομήτης was derived from κομᾶν (koman) 'to wear the hair long', which was itself derived from κόμη (komē) 'the hair of the head' and was used to mean 'the tail of a comet'.


The astronomical symbol for comets (represented in Unicode) is U+2604 ☄ COMET, consisting of a small disc with three hairlike extensions.


Physical characteristics


The solid, core structure of a comet is known as the nucleus. Cometary nuclei are composed of an amalgamation of rock, dust, water ice, and frozen carbon dioxide, carbon monoxide, methane, and ammonia. As such, they are popularly described as "dirty snowballs" after Fred Whipple's model. Comets with a higher dust content have been called "icy dirtballs". The term "icy dirtballs" arose after observation of Comet 9P/Tempel 1 collision with an "impactor" probe sent by NASA Deep Impact mission in July 2005. Research conducted in 2014 suggests that comets are like "deep fried ice cream", in that their surfaces are formed of dense crystalline ice mixed with organic compounds, while the interior ice is colder and less dense.


The surface of the nucleus is generally dry, dusty or rocky, suggesting that the ices are hidden beneath a surface crust several metres thick. In addition to the gases already mentioned, the nuclei contain a variety of organic compounds, which may include methanol, hydrogen cyanide, formaldehyde, ethanol, ethane, and perhaps more complex molecules such as long-chain hydrocarbons and amino acids. In 2009, it was confirmed that the amino acid glycine had been found in the comet dust recovered by NASA's Stardust mission. In August 2011, a report, based on NASA studies of meteorites found on Earth, was published suggesting DNA and RNA components (adenine, guanine, and related organic molecules) may have been formed on asteroids and comets.


The outer surfaces of cometary nuclei have a very low albedo, making them among the least reflective objects found in the Solar System. The Giotto space probe found that the nucleus of Halley's Comet (1P/Halley) reflects about four percent of the light that falls on it, and Deep Space 1 discovered that Comet Borrelly's surface reflects less than 3.0%; by comparison, asphalt reflects seven percent. The dark surface material of the nucleus may consist of complex organic compounds. Solar heating drives off lighter volatile compounds, leaving behind larger organic compounds that tend to be very dark, like tar or crude oil. The low reflectivity of cometary surfaces causes them to absorb the heat that drives their out-gassing processes.


Comet nuclei with radii of up to 30 kilometers (19 mi) have been observed, but ascertaining their exact size is difficult. The nucleus of 322P/SOHO is probably only 100–200 meters (330–660 ft) in diameter. A lack of smaller comets being detected despite the increased sensitivity of instruments has led some to suggest that there is a real lack of comets smaller than 100 meters (330 ft) across. Known comets have been estimated to have an average density of 0.6 g/cm3 (0.35 oz/cu in). Because of their low mass, comet nuclei do not become spherical under their own gravity and therefore have irregular shapes.


Roughly six percent of the near-Earth asteroids are thought to be the extinct nuclei of comets that no longer experience out-gassing, including 14827 Hypnos and 3552 Don Quixote.


Results from the Rosetta and Philae spacecraft show that the nucleus of 67P/Churyumov–Gerasimenko has no magnetic field, which suggests that magnetism may not have played a role in the early formation of planetesimals. Further, the ALICE spectrograph on Rosetta determined that electrons (within 1 km (0.62 mi) above the comet nucleus) produced from photoionization of water molecules by solar radiation, and not photons from the Sun as thought earlier, are responsible for the degradation of water and carbon dioxide molecules released from the comet nucleus into its coma. Instruments on the Philae lander found at least sixteen organic compounds at the comet's surface, four of which (acetamide, acetone, methyl isocyanate and propionaldehyde) have been detected for the first time on a comet.


The streams of dust and gas thus released form a huge and extremely thin atmosphere around the comet called the "coma". The force exerted on the coma by the Sun's radiation pressure and solar wind cause an enormous "tail" to form pointing away from the Sun.


The coma is generally made of water and dust, with water making up to 90% of the volatiles that outflow from the nucleus when the comet is within 3 to 4 astronomical units (450,000,000 to 600,000,000 km; 280,000,000 to 370,000,000 mi) of the Sun. The H2O parent molecule is destroyed primarily through photo-dissociation and to a much smaller extent photoionization, with the solar wind playing a minor role in the destruction of water compared to photo-chemistry. Larger dust particles are left along the comet's orbital path whereas smaller particles are pushed away from the Sun into the comet's tail by light pressure.


Although the solid nucleus of comets is generally less than 60 kilometers (37 mi) across, the coma may be thousands or millions of kilometers across, sometimes becoming larger than the Sun. For example, about a month after an outburst in October 2007, comet 17P/Holmes briefly had a tenuous dust atmosphere larger than the Sun. The Great Comet of 1811 also had a coma roughly the diameter of the Sun. Even though the coma can become quite large, its size can decrease about the time it crosses the orbit of Mars around 1.5 astronomical units (220,000,000 km; 140,000,000 mi) from the Sun. At this distance the solar wind becomes strong enough to blow the gas and dust away from the coma, and in doing so enlarging the tail. Ion tails have been observed to extend one astronomical unit (150 million km) or more.


Both the coma and tail are illuminated by the Sun and may become visible when a comet passes through the inner Solar System, the dust reflects sunlight directly while the gases glow from ionization. Most comets are too faint to be visible without the aid of a telescope, but a few each decade become bright enough to be visible to the naked eye. Occasionally a comet may experience a huge and sudden outburst of gas and dust, during which the size of the coma greatly increases for a period of time. This happened in 2007 to Comet Holmes.


In 1996, comets were found to emit X-rays. This greatly surprised astronomers because X-ray emission is usually associated with very high-temperature bodies. The X-rays are generated by the interaction between comets and the solar wind: when highly charged solar wind ions fly through a cometary atmosphere, they collide with cometary atoms and molecules, "stealing" one or more electrons from the atom in a process called "charge exchange". This exchange or transfer of an electron to the solar wind ion is followed by its de-excitation into the ground state of the ion by the emission of X-rays and far ultraviolet photons.


Bow shock


Bow shocks form as a result of the interaction between the solar wind and the cometary ionosphere, which is created by the ionization of gases in the coma. As the comet approaches the Sun, increasing out-gassing rates cause the coma to expand, and the sunlight ionizes gases in the coma. When the solar wind passes through this ion coma, the bow shock appears.


The first observations were made in the 1980s and 1990s as several spacecraft flew by comets 21P/Giacobini–Zinner, 1P/Halley, and 26P/Grigg–Skjellerup. It was then found that the bow shocks at comets are wider and more gradual than the sharp planetary bow shocks seen at, for example, Earth. These observations were all made near perihelion when the bow shocks already were fully developed.


The Rosetta spacecraft observed the bow shock at comet 67P/Churyumov–Gerasimenko at an early stage of bow shock development when the out-gassing increased during the comet's journey toward the Sun. This young bow shock was called the "infant bow shock". The infant bow shock is asymmetric and, relative to the distance to the nucleus, wider than fully developed bow shocks.


Tails


In the outer Solar System, comets remain frozen and inactive and are extremely difficult or impossible to detect from Earth due to their small size. Statistical detections of inactive comet nuclei in the Kuiper belt have been reported from observations by the Hubble Space Telescope but these detections have been questioned. As a comet approaches the inner Solar System, solar radiation causes the volatile materials within the comet to vaporize and stream out of the nucleus, carrying dust away with them.


The streams of dust and gas each form their own distinct tail, pointing in slightly different directions. The tail of dust is left behind in the comet's orbit in such a manner that it often forms a curved tail called the type II or dust tail. At the same time, the ion or type I tail, made of gases, always points directly away from the Sun because this gas is more strongly affected by the solar wind than is dust, following magnetic field lines rather than an orbital trajectory. On occasions—such as when Earth passes through a comet's orbital plane, the anti-tail, pointing in the opposite direction to the ion and dust tails, may be seen.


The observation of anti-tails contributed significantly to the discovery of solar wind. The ion tail is formed as a result of the ionization by solar ultra-violet radiation of particles in the coma. Once the particles have been ionized, they attain a net positive electrical charge, which in turn gives rise to an "induced magnetosphere" around the comet. The comet and its induced magnetic field form an obstacle to outward flowing solar wind particles. Because the relative orbital speed of the comet and the solar wind is supersonic, a bow shock is formed upstream of the comet in the flow direction of the solar wind. In this bow shock, large concentrations of cometary ions (called "pick-up ions") congregate and act to "load" the solar magnetic field with plasma, such that the field lines "drape" around the comet forming the ion tail.


If the ion tail loading is sufficient, the magnetic field lines are squeezed together to the point where, at some distance along the ion tail, magnetic reconnection occurs. This leads to a "tail disconnection event". This has been observed on a number of occasions, one notable event being recorded on 20 April 2007, when the ion tail of Encke's Comet was completely severed while the comet passed through a coronal mass ejection. This event was observed by the STEREO space probe.


In 2013, ESA scientists reported that the ionosphere of the planet Venus streams outwards in a manner similar to the ion tail seen streaming from a comet under similar conditions.


Jets


Uneven heating can cause newly generated gases to break out of a weak spot on the surface of comet's nucleus, like a geyser. These streams of gas and dust can cause the nucleus to spin, and even split apart. In 2010 it was revealed dry ice (frozen carbon dioxide) can power jets of material flowing out of a comet nucleus. Infrared imaging of Hartley 2 shows such jets exiting and carrying with it dust grains into the coma.


Orbital characteristics


Most comets are small Solar System bodies with elongated elliptical orbits that take them close to the Sun for a part of their orbit and then out into the further reaches of the Solar System for the remainder. Comets are often classified according to the length of their orbital periods: The longer the period the more elongated the ellipse.


Short period


Periodic comets or short-period comets are generally defined as those having orbital periods of less than 200 years. They usually orbit more-or-less in the ecliptic plane in the same direction as the planets. Their orbits typically take them out to the region of the outer planets (Jupiter and beyond) at aphelion; for example, the aphelion of Halley's Comet is a little beyond the orbit of Neptune. Comets whose aphelia are near a major planet's orbit are called its "family". Such families are thought to arise from the planet capturing formerly long-period comets into shorter orbits.


At the shorter orbital period extreme, Encke's Comet has an orbit that does not reach the orbit of Jupiter, and is known as an Encke-type comet. Short-period comets with orbital periods less than 20 years and low inclinations (up to 30 degrees) to the ecliptic are called traditional Jupiter-family comets (JFCs). Those like Halley, with orbital periods of between 20 and 200 years and inclinations extending from zero to more than 90 degrees, are called Halley-type comets (HTCs). As of 2022, 94 HTCs have been observed, compared with 744 identified JFCs.


Recently discovered main-belt comets form a distinct class, orbiting in more circular orbits within the asteroid belt.


Because their elliptical orbits frequently take them close to the giant planets, comets are subject to further gravitational perturbations. Short-period comets have a tendency for their aphelia to coincide with a giant planet's semi-major axis, with the JFCs being the largest group. It is clear that comets coming in from the Oort cloud often have their orbits strongly influenced by the gravity of giant planets as a result of a close encounter. Jupiter is the source of the greatest perturbations, being more than twice as massive as all the other planets combined. These perturbations can deflect long-period comets into shorter orbital periods.


Based on their orbital characteristics, short-period comets are thought to originate from the centaurs and the Kuiper belt/scattered disc—a disk of objects in the trans-Neptunian region—whereas the source of long-period comets is thought to be the far more distant spherical Oort cloud (after the Dutch astronomer Jan Hendrik Oort who hypothesized its existence). Vast swarms of comet-like bodies are thought to orbit the Sun in these distant regions in roughly circular orbits. Occasionally the gravitational influence of the outer planets (in the case of Kuiper belt objects) or nearby stars (in the case of Oort cloud objects) may throw one of these bodies into an elliptical orbit that takes it inwards toward the Sun to form a visible comet. Unlike the return of periodic comets, whose orbits have been established by previous observations, the appearance of new comets by this mechanism is unpredictable. When flung into the orbit of the sun, and being continuously dragged towards it, tons of matter are stripped from the comets which greatly influence their lifetime; the more stripped, the shorter they live and vice versa.


Long period


Long-period comets have highly eccentric orbits and periods ranging from 200 years to thousands or even millions of years. An eccentricity greater than 1 when near perihelion does not necessarily mean that a comet will leave the Solar System. For example, Comet McNaught had a heliocentric osculating eccentricity of 1.000019 near its perihelion passage epoch in January 2007 but is bound to the Sun with roughly a 92,600-year orbit because the eccentricity drops below 1 as it moves farther from the Sun. The future orbit of a long-period comet is properly obtained when the osculating orbit is computed at an epoch after leaving the planetary region and is calculated with respect to the center of mass of the Solar System. By definition long-period comets remain gravitationally bound to the Sun; those comets that are ejected from the Solar System due to close passes by major planets are no longer properly considered as having "periods". The orbits of long-period comets take them far beyond the outer planets at aphelia, and the plane of their orbits need not lie near the ecliptic. Long-period comets such as C/1999 F1 and C/2017 T2 (PANSTARRS) can have aphelion distances of nearly 70,000 AU (0.34 pc; 1.1 ly) with orbital periods estimated around 6 million years.


Single-apparition or non-periodic comets are similar to long-period comets because they also have parabolic or slightly hyperbolic trajectories when near perihelion in the inner Solar System. However, gravitational perturbations from giant planets cause their orbits to change. Single-apparition comets have a hyperbolic or parabolic osculating orbit which allows them to permanently exit the Solar System after a single pass of the Sun. The Sun's Hill sphere has an unstable maximum boundary of 230,000 AU (1.1 pc; 3.6 ly). Only a few hundred comets have been seen to reach a hyperbolic orbit (e > 1) when near perihelion that using a heliocentric unperturbed two-body best-fit suggests they may escape the Solar System.


As of 2022, only two objects have been discovered with an eccentricity significantly greater than one: 1I/ʻOumuamua and 2I/Borisov, indicating an origin outside the Solar System. While Oumuamua, with an eccentricity of about 1.2, showed no optical signs of cometary activity during its passage through the inner Solar System in October 2017, changes to its trajectory—which suggests out-gassing—indicate that it is probably a comet. On the other hand, 2I/Borisov, with an estimated eccentricity of about 3.36, has been observed to have the coma feature of comets, and is considered the first detected interstellar comet. Comet C/1980 E1 had an orbital period of roughly 7.1 million years before the 1982 perihelion passage, but a 1980 encounter with Jupiter accelerated the comet giving it the largest eccentricity (1.057) of any known solar comet with a reasonable observation arc.[105] Comets not expected to return to the inner Solar System include C/1980 E1, C/2000 U5, C/2001 Q4 (NEAT), C/2009 R1, C/1956 R1, and C/2007 F1 (LONEOS).


Some authorities use the term "periodic comet" to refer to any comet with a periodic orbit (that is, all short-period comets plus all long-period comets), whereas others use it to mean exclusively short-period comets. Similarly, although the literal meaning of "non-periodic comet" is the same as "single-apparition comet", some use it to mean all comets that are not "periodic" in the second sense (that is, to also include all comets with a period greater than 200 years).


Early observations have revealed a few genuinely hyperbolic (i.e. non-periodic) trajectories, but no more than could be accounted for by perturbations from Jupiter. Comets from interstellar space are moving with velocities of the same order as the relative velocities of stars near the Sun (a few tens of km per second). When such objects enter the Solar System, they have a positive specific orbital energy resulting in a positive velocity at infinity ( v ∞ {\displaystyle v_{\infty }\!}) and have notably hyperbolic trajectories. A rough calculation shows that there might be four hyperbolic comets per century within Jupiter's orbit, give or take one and perhaps two orders of magnitude.


Oort cloud and Hills cloud


The Oort cloud is thought to occupy a vast space starting from between 2,000 and 5,000 AU (0.03 and 0.08 ly) to as far as 50,000 AU (0.79 ly) from the Sun. This cloud encases the celestial bodies that start at the middle of our solar system—the sun, all the way to outer limits of the Kuiper Belt. The Oort cloud consists of viable materials necessary for the creation of celestial bodies. The planets we have today, exist only because of the planetesimals (chunks of leftover space that assisted in the creation of planets) that were condensed and formed by the gravity of the sun. The eccentric made from these trapped planetesimals is why the Oort Cloud even exists. Some estimates place the outer edge at between 100,000 and 200,000 AU (1.58 and 3.16 ly). The region can be subdivided into a spherical outer Oort cloud of 20,000–50,000 AU (0.32–0.79 ly), and a doughnut-shaped inner cloud, the Hills cloud, of 2,000–20,000 AU (0.03–0.32 ly). The outer cloud is only weakly bound to the Sun and supplies the long-period (and possibly Halley-type) comets that fall to inside the orbit of Neptune. The inner Oort cloud is also known as the Hills cloud, named after J. G. Hills, who proposed its existence in 1981. Models predict that the inner cloud should have tens or hundreds of times as many cometary nuclei as the outer halo; it is seen as a possible source of new comets that resupply the relatively tenuous outer cloud as the latter's numbers are gradually depleted. The Hills cloud explains the continued existence of the Oort cloud after billions of years.


Exocomets


Exocomets beyond the Solar System have also been detected and may be common in the Milky Way. The first exocomet system detected was around Beta Pictoris, a very young A-type main-sequence star, in 1987. A total of 11 such exocomet systems have been identified as of 2013, using the absorption spectrum caused by the large clouds of gas emitted by comets when passing close to their star. For ten years the Kepler space telescope was responsible for searching for planets and other forms outside of the solar system. The first transiting exocomets were found in February 2018 by a group consisting of professional astronomers and citizen scientists in light curves recorded by the Kepler Space Telescope. After Kepler Space Telescope retired in October 2018, a new telescope called TESS Telescope has taken over Kepler's mission. Since the launch of TESS, astronomers have discovered the transits of comets around the star Beta Pictoris using a light curve from TESS. Since TESS has taken over, astronomers have since been able to better distinguish exocomets with the spectroscopic method. New planets are detected by the white light curve method which is viewed as a symmetrical dip in the charts readings when a planet overshadows its parent star. However, after further evaluation of these light curves, it has been discovered that the asymmetrical patterns of the dips presented are caused by the tail of a comet or of hundreds of comets.


Effects of comets


As a comet is heated during close passes to the Sun, out-gassing of its icy components also releases solid debris too large to be swept away by radiation pressure and the solar wind. If Earth's orbit sends it through that trail of debris, which is composed mostly of fine grains of rocky material, there is likely to be a meteor shower as Earth passes through. Denser trails of debris produce quick but intense meteor showers and less dense trails create longer but less intense showers. Typically, the density of the debris trail is related to how long ago the parent comet released the material. The Perseid meteor shower, for example, occurs every year between 9 and 13 August, when Earth passes through the orbit of Comet Swift–Tuttle. Halley's Comet is the source of the Orionid shower in October.

 

FLOTUS: Dolley Madison




Dolley Todd Madison (née Payne; May 20, 1768 – July 12, 1849) was the wife of James Madison, the fourth president of the United States from 1809 to 1817. She was noted for holding Washington social functions in which she invited members of both political parties, essentially spearheading the concept of bipartisan cooperation. Previously, founders such as Thomas Jefferson would only meet with members of one party at a time, and politics could often be a violent affair resulting in physical altercations and even duels. Madison helped to create the idea that members of each party could amicably socialize, network, and negotiate with each other without violence. By innovating political institutions as the wife of James Madison, Dolley Madison did much to define the role of the President's spouse, known only much later by the title first lady—a function she had sometimes performed earlier for the widowed Thomas Jefferson.


Madison also helped to furnish the newly constructed White House. When the British set fire to it in 1814, she was credited with saving Gilbert Stuart's classic 1796 portrait of George Washington; she directed her personal slave Paul Jennings to save it. In widowhood, she often lived in poverty aggravated by her son John Payne Todd's alcoholism and mismanagement of their Montpelier plantation. To relieve her debts, she sold off the plantation, its remaining slaves, and her late husband's papers.


Surveys of historians conducted periodically by the Siena College Research Institute since 1982 have consistently found Madison to rank among the six most highly regarded first ladies by the assessments of historians.


Early life and first marriage


Madison was born as Dolley Payne on May 20, 1768, in a log cabin in New Garden, Guilford County (present-day Greensboro), North Carolina, to Mary Coles and John Payne Jr. Her parents had married in 1761, uniting two prominent Virginian families. Little is known about the family's life before 1793, when Madison was 25, because few documents have survived; Madison's earliest known letter dates to 1783. Mary Coles was from a Quaker family and two years after their marriage the couple applied for membership in the Ceder Creek meeting. The application was considered for a very lengthy time before they were admitted in 1765. He would become a fervent member of the faith. The family had moved to New Garden, a Quaker community, in 1765. Madison was the family's third child and first daughter. The family had an enslaved nursemaid.


In early 1769, the Paynes returned to Virginia for reasons that are unclear. Historians Catherine Allgor and Richard N. Côté have speculated in their biographical works on her that the family may have wanted to return to their extended family, become uncomfortable with the religion, faced local opposition, or failed at farming or business. Madison would later downplay her North Carolina birth, claiming herself to be a Virginian born when visiting an uncle in North Carolina. The family returned to Cedar Creek, where within four years they had moved at least twice. They eventually settled on a 176 acres (71 ha) farm several miles outside of Scotchtown. Madison grew up on the farm, working the land with the rest of her family. She was given a strict Quaker upbringing and education, which Côté describes her as "chafing" under.


Madison grew close to her extended family in the area. She had three younger sisters (Lucy, Anna, and Mary) and four brothers (Walter, William Temple, Isaac, and John), two of whom were younger. Her father did not participate in the American Revolutionary War, as his faith practiced pacifism, and Allgor writes that Madison was seemingly little affected by it. By 1783 John Payne had emancipated his slaves, as did numerous slaveholders in the Upper South. Payne, as a Quaker, had long encouraged manumission, but the act was not legal in Virginia until 1782.


When Madison was 15, Payne moved his family to Philadelphia, at the time the second largest American city. They lived at 57 North Third Street, and transferred to the local Northern District Meeting. While living there, Madison often visited Haddonfield, New Jersey, where many Quakers lived. She also met Eliza Collins and Dorothea Abrahams in Philadelphia, with whom she became lifelong friends. During her early years, Payne likely received formal education, though it is not known what this was. Allgor concludes that it was likely better than most Americans at the time, while Côté notes that it was probably "no more than a basic" one. Madison grew into a young woman who Côté writes was described "as one of the fairest of the fair".


Upon the family's move to Philadelphia, John had attempted to build a career as a starch manufacturer, but the business failed in 1789. This was seen as a "weakness" at his Quaker meetings, for which he was expelled. He was devastated by this failure and died on October 24, 1792. Mary Payne initially made ends meet by opening her home as a boardinghouse beginning in 1791. Before his death, John had arranged Madison's marriage to John Todd, a Philadelphia lawyer. According to Allgor, Madison had rejected marriage with Todd previously and John's marriage arrangement was "manipulation". Conversely, Côté considers their marriage to have been "for love, not just duty". They were married on January 7, 1790, at a Quaker meeting house. Madison's friend Eliza Collins was her bridesmaid. The couple moved several blocks away into a high-quality neighborhood.


Marriage and family


Madison and Todd had two sons, John Payne (called Payne, born February 29, 1792) and William Temple (born July 4, 1793). According to Allgor, their marriage grew into a "a loving happy partnership." Madison's sister Anna Payne moved in with them.


In August 1793, a yellow fever epidemic broke out in Philadelphia, killing 5,019 people in four months. Madison was hit particularly hard, losing her husband, son William, mother-in-law, and father-in-law. Two of her older brothers died just two years later, and Côté writes that she was "never fully recovered" from the emotional toll of these deaths.


While undergoing the loss of much of her family, she also had to take care of her surviving son without financial support. While her husband had left her money in his will, the executor, her brother-in-law, withheld the funds and she sued him for what she was owed. Aaron Burr, who had once stayed at the boarding house of Madison's mother, assisted her in these efforts, offering legal advice. In a will, written around that time, Burr was named the guardian of Madison's only surviving child.


Second marriage


Madison, at the time named Dolley Todd, soon met James Madison. Their relationship was facilitated by Burr, a longtime friend of Madison. In May 1794, Burr made the formal introduction between the young widow and Madison, who at 43 was a longstanding bachelor 17 years her senior. A brisk courtship followed and, by August, Dolley Madison accepted his marriage proposal. As he was not a Quaker, she was expelled from the Society of Friends for marrying outside her faith, after which Dolley Madison began attending Episcopal services. Despite her Quaker upbringing, there is no evidence that she disapproved of James as a slaveholder. They were married on September 15, 1794, and lived in Philadelphia for the next three years.


In 1797, after eight years in the House of Representatives, James Madison retired from politics. He returned with his family to Montpelier, the Madison family plantation in Orange County, Virginia. There they expanded the house and settled in. When Thomas Jefferson was elected as the third president of the United States in 1800, he asked James Madison to serve as his secretary of state. James Madison accepted and moved with Dolley Madison, her son Payne, her sister Anna, and their domestic slaves to Washington on F Street. They took a large house, as Dolley Madison believed that entertaining would be important in the new capital.


In Washington 1801–1817


Madison worked with the architect Benjamin Henry Latrobe to furnish the White House, the first official residence built for the president of the United States. She sometimes served as widower Jefferson's hostess for official ceremonial functions. Madison would become a crucial part of the Washington social circle, befriending the wives of numerous diplomats like Sarah Martinez de Yrujo, wife of the ambassador of Spain, and Marie-Angelique Turreau, the wife of the French ambassador. Her charm precipitated a diplomatic crisis, called the Merry Affair, after Jefferson escorted Madison to the dining room instead of the wife of Anthony Merry, English diplomat to the U.S., in a major faux pas.


In the approach to the 1808 presidential election, with Thomas Jefferson ready to retire, the Democratic-Republican caucus nominated James Madison to succeed him. He was elected the fourth President of the United States, serving two terms from 1809 to 1817, and Madison became the official White House hostess. Madison had often been the unofficial hostess at the White House during Jefferson's presidency. While the term "first lady" was not yet in use. Madison's role as hostess became official when her own husband assumed the presidency. Madison helped to define the official functions, decorated the Executive Mansion, and welcomed visitors in her drawing room. She was renowned for her social graces and hospitality, and contributed to her husband's popularity as president. She was the only First Lady given an honorary seat on the floor of Congress, and the first American to respond to a telegraph message. In 1812, James was re-elected. Later that year, he delivered a war request to Congress, signaling the beginning of the War of 1812.


Burning of Washington, 1814


After the United States declared war in 1812 and attempted to invade Canada in 1813, a British force attacked Washington in 1814. As it approached and the White House staff hurriedly prepared to flee, Madison ordered her personal slave Paul Jennings to save the Stuart painting, a copy of the Lansdowne portrait, as she wrote in a letter to her sister at 3 o'clock in the afternoon of August 23:


Our kind friend Mr. Carroll has come to hasten my departure, and in a very bad humor with me, because I insist on waiting until the large picture of General Washington is secured, and it requires to be unscrewed from the wall. The process was found too tedious for these perilous moments; I have ordered the frame to be broken and the canvas taken out ... It is done, and the precious portrait placed in the hands of two gentlemen from New York for safe keeping. On handing the canvas to the gentlemen in question, Messrs. Barker and Depeyster, Mr. Sioussat cautioned them against rolling it up, saying that it would destroy the portrait. He was moved to this because Mr. Barker started to roll it up for greater convenience for carrying.


Popular accounts during and after the war years tended to portray Madison as the one who removed the painting, and she became a national heroine. An 1865 memoir by Jennings stated that she had ordered him to save the painting, and that Jean Pierre Sioussat and a gardener, McGraw, were the ones to remove it from the wall. Early twentieth-century historians noted that Sioussat had directed the servants, many of whom were slaves, in the crisis, and that house slaves were the ones who actually preserved the painting.


Dolley Madison hurried away in her waiting carriage, along with other families fleeing the city. They went to Georgetown and the next day they crossed over the Potomac into Virginia. When the couple returned to Washington, the White House was uninhabitable and Dolley and James Madison moved into The Octagon House.


In Montpelier 1817–1837


On April 6, 1817, a month after his retirement from the presidency, Dolley and James Madison returned to the Montpelier plantation in Orange County, Virginia.


In 1830, Madison's son Payne Todd, who had never found a career, went to debtors' prison in Philadelphia and the Madisons sold land in Kentucky and mortgaged half of the Montpelier plantation to pay his debts.


James died at Montpelier on June 28, 1836. He was 85 years old. Madison remained at Montpelier for a year. Her niece Anna Payne moved in with her, and Todd came for a lengthy stay. During this time, Madison organized and copied her husband's papers. Congress authorized $55,000 as payment for editing and publishing seven volumes of the Madison papers, including his unique notes on the 1787 convention.


In the fall of 1837, Madison returned to Washington, charging Todd with the care of the plantation. She and her sister Anna moved into a house, bought by Anna and her husband Richard Cutts, on Lafayette Square. Madison took Paul Jennings with her as a butler, and he was forced to leave his wife and children in Virginia.


In Washington 1837–1849


While Dolley Madison was living in Washington, Payne Todd was unable to manage the plantation, due to alcoholism and related illness. She tried to raise money by selling the rest of the president's papers, but was unable to find a buyer. Jennings attempted to negotiate purchasing his freedom; she had previously written a will in 1841 which would free Jennings after her death, though not her other slaves. She instead sold him to an insurance agent for $200 in 1846. Six months later, Senator Daniel Webster intervened to buy him from the new owner and gave Jennings his freedom, for which he repaid the senator in work. Madison sold Montpelier, its remaining slaves, and the furnishings to pay off outstanding debts. Jennings later recalled in his memoir,


In the last days of her life, before Congress purchased her husband's papers, she was in a state of absolute poverty, and I think sometimes suffered for the necessaries of life. While I was a servant to Mr. Webster, he often sent me to her with a market-basket full of provisions, and told me whenever I saw anything in the house that I thought she was in need of, to take it to her. I often did this, and occasionally gave her small sums from my own pocket, though I had years before bought my freedom of her.


In 1848, Congress agreed to buy the rest of James Madison's papers for the sum of $22,000 or $25,000.


In 1845, Dolley Madison was baptized into St. John's Episcopal Church, Lafayette Square in Washington, D.C.


On February 28, 1844, Madison was with President John Tyler while aboard the USS Princeton when a "Peacemaker" cannon exploded in the process of being fired. While Secretaries of State and Navy Abel P. Upshur and Thomas Walker Gilmer, Tyler's future father-in-law David Gardiner and three others were killed, Tyler and Madison escaped unharmed.


She was photographed on at least two occasions, making her the earliest First Lady to have a surviving photograph, with four daguerreotypes known to survive as of 2021. Three photographs were taken on July 4, 1848, including one featuring her niece, Anna Payne; the final one was taken in 1849, featuring President James Polk, his wife Sarah Polk, future President James Buchanan and future First Lady Harriet Lane.


Dolley Madison died at her home in Washington in 1849, at the age of 81. She was first buried in the Congressional Cemetery, Washington, D.C., but later was re-interred at Montpelier next to her husband. She was buried in an air-tight Fisk metallic burial case with a glass window plate for viewing the face of the deceased.


Honors


Madison (second to right) on the portico of the White House alongside Secretary of State James Buchanan, future First Lady Harriet Lane, president James Polk and his wife, Sarah.


During World War II the Liberty ship SS Dolly Madison was built in Panama City, Florida, and named in her honor.


Madison was a member of the inaugural class of Virginia Women in History in 2000.


Spelling of her name


In the past, biographers and others stated that her given name was Dorothea, after her aunt, or Dorothy, and that Dolley was a nickname. But her birth was registered with the New Garden Friends Meeting as Dolley, and her will of 1841 states "I, Dolly P. Madison". Based on manuscript evidence and the scholarship of recent biographers, Dollie, spelled "i.e.", appears to have been her given name at birth. On the other hand, the print press, especially newspapers, tended to spell it "Dolly": for example, the Hallowell (Maine) Gazette, February 8, 1815, p. 4, refers to how the Congress had allowed "Madame Dolly Madison" an allowance of $14,000 to purchase new furniture; and the New Bedford (MA) of March 3, 1837, p. 2 referred to a number of important papers from her late husband, and said that "Mrs. Dolly Madison" would be paid by the Senate for these historical manuscripts. Several magazines of that time also used the "Dolly" spelling, such as The Knickerbocker, February 1837, p. 165; as did many popular magazines of the 1860s–1890s. She was referred to as "Mistress Dolly" in an essay from Munsey's Magazine in 1896. Her grandniece Lucia Beverly Cutts, in her Memoirs and letters of Dolly Madison: wife of James Madison, president of the United States (1896) uses "Dolly" consistently throughout.


Representation in other media


Cecil B. DeMille, The Buccaneer, 1938 film, played by Spring Byington


Irving Stone, Magnificent Doll (1946), film directed by Frank Borzage, Universal Pictures


Brown, Rita Mae, Dolley: A Novel of Dolley Madison in Love and War, New York: Bantam Books, 1994; reprint (Presidential Wives Series), Huntington, NY: Nova History Publications, 2001


1999 Dolley Madison commemorative silver dollar


Legacy


Virginia State Route 123 is named Dolley Madison Boulevard from McLean, Virginia to George Washington Memorial Parkway.


Regard by historians


Since 1982 Siena College Research Institute has periodically conducted surveys asking historians to assess American first ladies according to a cumulative score on the independent criteria of their background, value to the country, intelligence, courage, accomplishments, integrity, leadership, being their own women, public image, and value to the president. Consistently, Madison has ranked among the six-most highly regarded first ladies in these surveys. In terms of cumulative assessment, Madison has been ranked:


4th-best of 42 in 1982

4th-best of 37 in 1993

3rd-best of 38 in 2003

6th-best of 38 in 2008

4th-best of 39 in 2014


In the 2008 Siena Research Institute survey, Madison was ranked in the top-four of all criteria, ranking the 4th-highest in value to the country and 5th-highest in public image. In the 2014 survey, Madison and her husband were ranked the 5th-highest out of 4th first couples in terms of being a "power couple".