Contents

List of former planets

Throughout antiquity, several astronomical objects were considered Classical Planets, meaning "wandering stars", not all of which are now considered planets. The moons discovered around Jupiter, Saturn and Uranus after the advent of the telescope were also initially considered planets by some. The development of more powerful telescopes resulted in the discovery of the asteroids, which were initially considered planets. Then Pluto, the first Trans-Neptunian Object, was discovered. More Trans-Neptunian Objects of the Kuiper Belt were found with the help of electronic imaging. One of these, Eris, was widely hailed as a "new planet", which prompted the 2006 recategorization of solar system bodies.

Some planetary scientists reject the 2006 definition of planet, and thus would still consider some of the objects on this list to be planets under a geophysical definition. See the list of gravitationally rounded objects of the Solar System for a list of geophysical planets.

List[edit]

Former planets of the Solar System

	Former planet	Discovery	Removal	Current status		Notes
	The Morning Star[NB 1]	Antiquity	Antiquity	Aspects of Venus		"Phosphorus", the Morning Star of Greek antiquity (Eosphorus, the Dawn-Bringer; called "Lucifer" by the Romans), and "Hesperus", the Evening Star (called "Vesper" by the Romans), were later identified as a single planet, Venus (Aphrodite).	[2][3]
	The Evening Star[NB 1]	Antiquity	Antiquity
	Apollo[NB 2]	Antiquity	Antiquity	Aspect of Mercury		Like the Morning and Evening Stars, Mercury was deemed to be a distinct planet when it was visible during daytime, and dedicated to Apollo by the Greeks. Eventually, in the 4th century BC, Mercury and Apollo were found to be one and the same.	[4]
	Sun	Antiquity	1543	Star		In antiquity, it was believed that the Sun and all the planets orbit the Earth. Thus the Sun was categorised as a planet. Following the acceptance of the Copernican model, it was recognized that the planets (including Earth) orbit the Sun, and it was no longer regarded as a planet. Subsequent discoveries show that the Sun is a star.	[5][6][7]
	Moon	Antiquity	1543	MoonofEarth		Following the acceptance of the Copernican model, planets were defined as objects which orbit the Sun. Since the Moon can be said to orbit the Earth, it was no longer regarded as a planet, but this is debated; see double planet.	[5][6][7]
	Io	1610	1700s	Moons of Jupiter		Originally presented as satellite planets orbiting the planet Jupiter. Planetary status later rescinded, leaving them only as satellites. Ganymede is the largest satellite in the Solar System, and is slightly larger than Mercury, but is about half as massive.	[8][9][10] [11][6][7]
	Europa	1610	1700s
	Ganymede	1610	1700s
	Callisto	1610	1700s
	Titan	1656	1700s	Moons of Saturn		Originally presented as satellite planets orbiting the planet Saturn. Planetary status later rescinded, leaving them only as satellites. Titan is the second largest satellite in the Solar System, and is slightly larger than Mercury, but less massive.	[12][6][7]
	Iapetus	1671	1700s				[13][11] [6][7]
	Rhea	1672	1700s
	Tethys	1684	1700s				[14][11] [6][7]
	Dione	1684	1700s
	Titania	1787	1700s	Moons of Uranus		Originally presented as satellite planets orbiting the planet Uranus.[15] Planetary status later rescinded, leaving them only as satellites.
	Oberon	1787	1700s
	Ceres	1801	1867	Asteroid and dwarf planet		The first asteroids to be discovered were accepted as planets in the Copernican system, since they directly orbited the Sun. By 1855 the number of known bodies in the asteroid belt had grown to 15, at which point astronomers started distinguishing these from the eight known major planets. The 1867 edition of Berliner Astronomisches Jahrbuch placed all the new bodies in the asteroid belt into a separate category as 'minor planets' or 'asteroids', by which point almost 100 asteroids had been observed.[16]	[17][18]
	Pallas	1802	1867	Asteroid
	Juno	1804	1867
	Vesta	1807	1867
	Astraea	1845	1867
	Hebe	1847	1867
	Iris	1847	1867
	Chiron	1977	1980	Centaur		The discovery of Chiron was hailed by the press and astrologers as that of a new planet. Astronomically, it was different from any other planets, asteroids and comets known at the time, and it was classified as unique at that time. Later it was called an asteroid, and then was found to exhibit characteristics of a comet, leading to multiple classifications. Later it was placed into its own category of centaurs, and many other centaurs have been discovered subsequently.	[19][20][21] [22][23]
	Pluto	1930	2006	Dwarf planet		Following its discovery in 1930, Pluto was widely regarded as the ninth planet. Numerous scientific discoveries cast doubt on this classification, and after the discovery of Eris, which was larger than Pluto, the International Astronomical Union met to determine a definition of planet. Like the asteroids before them, Pluto was grouped together with Eris and similar bodies as members of a group of smaller objects designated as dwarf planets.	[24][25]
	Charon	1978	2006	Moon of Pluto		When discovered, Charon, the moon of Pluto, was found to be very large, leading to the declaration by many that the Pluto-Charon system was a double planet (binary planet). The 2006 IAU redefinition of planet excludes the possibility of double planets.	[24][25][26]
	15760 Albion	1992	unknown	Trans-Neptunian object		When discovered, these bodies were briefly hailed as the tenth and eleventh planets by the press, but it was then decided that 15760 Albion was the prototype of trans-Neptunian objectsorcubewanos.	[27][28]
	(181708) 1993 FW	1992	unknown				[28]
	Eris	2005	2006	Dwarf planet		The discovery of Eris, hailed worldwide by the press as the tenth planet, prompted the International Astronomical Union to meet and establish a new definition of planet. It was recategorised as a dwarf planet, together with Pluto and numerous other objects.	[25][29]

See also[edit]

• List of gravitationally rounded objects of the Solar System
• List of possible dwarf planets
• List of hypothetical Solar System objects

Notes[edit]

References[edit]

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