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Science Astronomy Planets (1) Planets Dwarf Planets Satellites (Moons)

Astronomy: Planets (1)

This page lists the basic characteristics of the planets and other major bodies of the Solar System.  For details of their atmosphere, surface and interior structure, see Planets (2).  For anything else, see Solar System.

Planets

... in order of the radii of their orbits around the Sun – in other words, their distances from the Sun:

Name Discovered By Relative Mass Diameter (miles) Mean radius of orbit (AU) Rotational period ('day') Orbital period ('year') Satellites (according to NASA, May 2025)
Mercury Known since ancient times 0.056 3,030 0.39 59 88 daysNone
Venus 0.82 7,500 0.72 243 225 daysNone
Earth 1 7,923 1 1 365.24 daysThe Moon (see below)
Mars 0.11 4,210 1.52 1.02 687 daysPhobos, Deimos (see below)
Jupiter 318 88,700 5.20 9hr 51min 11.86 years 97 (Ganymede is the largest)
Saturn 95 75,000 9.54 10hr 14m 29.46 years 274 (Titan is the largest)
Uranus1781 William Herschel 14.5 31,600 19.22 17hrs 24min 84 years28 (named after Shakespearean characters)
Neptune1846 J. G. Galle 17.2 30,200 30.06 16hr 7min 164.8 years16 (2 are visible from Earth)

Twelve new moons of Jupiter were discovered in July 2018.

The four largest moons of Jupiter (Io, Europa, Ganymede and Callisto) were discovered in 1610 by Galileo Galilei and are known as the Galilean satellites. They were the first celestial objects to be discovered by telescope.

Dwarf planets

The term 'dwarf planet' was coined in 1990 by the American planetary scientist Alan Stern, and the concept was adopted by the IAU in 2006. A dwarf planet is defined (on Wikipedia) as "a small planetary–mass object that is in direct orbit around the Sun, massive enough to be gravitationally rounded, but insufficient to achieve orbital dominance like the eight classical planets of the Solar System."

Pluto, discovered in 1930 and previously considered a planet, was 'demoted' in 2006 to become one of the first three dwarf planets, which are:

Name Discvrd By Mass (kg) Diameter (km) Mean radius of orbit (AU) Rotational period ('day') Orbital period ('year') Satellites
Ceres1801 Giuseppe Piazzi 9.38 x 1020 939.4 2.77 9.1 hours 1,680 daysNone
Pluto1930 Clyde Tombaugh 13 x 1021 2,377 39.48 6.39 days 248.5 yearsCharon (see below), Styx, Nix, Kerberos, Hydra
Eris2003 Mike Brown 16.47 x 1021 2,326 67.86 15 days 18.9 hrs 559 yearsDysnomia

The following are "generally assumed to be dwarf planets" (according to Wikipedia):

Makemake 2004 Mike Brown 3.1 x 1021 1,430 45.56 22.8 hours 307.5 years One (no informal name)
Haumea 2005 Mike Brown 4.01 x 1021 1,560 43.22 3.9 hours 284.1 yearsHi'iaka, Namaka

Haumea has one known ring.

The following "meet the preliminary criteria ... for identifying dwarf planets, and are generally called dwarf planets by astronomers as well":

Quaoar 2002 Trujillo & Brown 1.2 x 1021 1,086 43.7 17.7 hours 288.8 years Weywot
Sedna 2003 Trujillo, Brown, Rabinovitz 1 x 1021? 906 506.8 10 hours 11,400 years None known
Orcus 2004 5.55 x 1020 910 39.4 13 hours 247.3 years Vanth
Gonggong 2007 Schwamb, Brown, Rabinowitz 1.75 x 1021 1,230 67.49 22.4 hours 554.4 years Xiangliu

Quaoar has two known rings.

These details were last updated in May 2025.

Satellites (Moons)

This section lists the ten most significant satellites or moons in the Solar System (the ones you're most likely to get asked about in a quiz.) For which satellite belongs to which planet, see the Planets table above. But for the record: Titan belongs to Saturn, and the other four biggest ones (other than The Moon) belong to Jupiter; Triton belongs to Neptune, Charon belongs to Pluto, and Phobos and Deimos both belong to Mars.

Name Discovered By Relative Mass Diameter (miles) Mean radius of orbit (miles) Rotational period ('day') Orbital period ('year') Satellites
Ganymede1610Galileo Galilei 0.0253,270 700,000Synchronous 7.2 daysThe ninth largest object in the solar system
Titan1655Christiaan Huygens 0.0233,200 759,000Synchronous 15.95 daysThe only 'moon' with an atmosphere (nitrogen)
Callisto1610Galileo 0.0183,000 1,170,100Synchronous 16.7 days
Io1610Galileo 0.0152,250 262,100Synchronous 1.8 days
The Moon 0.0122,160 238,855Synchronous 27.32 days *
Europa1610Galileo 0.0081,950 417,000Synchronous 3.6 days
Triton1846William Lasell 0.00361,680 220,400Synchronous –5.877 daysThe only large moon with a retrograde orbit
Charon1978James W. Christy 3 * 10–51,200 12,500Synchronous 6.39 days
Phobos1877Asaph Hall (US) 5.6 * 10–917 5,840Synchronous 0.32 daysIrregularly shaped – diameter given is largest
Deimos1877Asaph Hall (US) 3.8 * 10–109 15,000Synchronous 1.26 daysIrregularly shaped – diameter given is largest

* 27 days, 7 hours, 41 minutes. The 'lunation period' – the time taken to complete the lunar cycle of phases – is 29.53 days

© Haydn Thompson 2017–25