Ceres (dwarf planet)

Ceres
Ceres as imaged by Dawn, May 2015. The two bright spots are the crater Haulani (right), and the floor of the crater Oxo (left).
Discovery
Discovered byGiuseppe Piazzi
Discovery date1 January 1801
Designations
Pronunciation/ˈsɪəriːz/, SEER-eez
Named after
Cerēs
(1) Ceres
AdjectivesCererian, -ean (/sɪˈrɪəriən/)
Symbol⚳
Orbital characteristics
Epoch 21 January 2022 (JD 2459600.5)
Aphelion2.98 AU (446 million km)
Perihelion2.55 AU (381 million km)
2.77 AU (414 million km)
Eccentricity0.0785
  • 4.60 yr
  • 1680 d
17.9 km/s
291.4°
Inclination
80.3°
7 December 2022
73.6°
SatellitesDawn (derelict space probe)
Proper orbital elements
2.77 AU
0.116
9.65°
78.2 deg / yr
4.60358 yr
(1681.458 d)
Precession of perihelion long.
54.1 arcsec / yr
Precession of asc. node
−59.2 arcsec / yr
Physical characteristics
Dimensions(966.2 × 962.0 × 891.8)
± 0.2 km
469.7±0.1 km (291.9 mi)
2,772,368 km2
Volume434,000,000 km3
Mass
  • (9.38392±0.00005)×1020 kg
  • 0.00016 Earths
  • 0.0128 Moons
Mean density
2.1616±0.0025 g/cm3
Equatorial surface gravity
0.284 m/s2 (0.0290 g0)
0.36±0.15 (estimate)
Equatorial escape velocity
0.516 km/s 1141 mph
9.074170±0.000001 h
Equatorial rotation velocity
92.61 m/s
≈4°
North pole right ascension
291.42744°
North pole declination
66.76033°
0.090±0.0033 (V-band)
Surface temp. min mean max
Kelvin ≈110 172.5±2 235±4
C
  • 7.6
  • 9.27 (July 2021)
3.35
0.854″ to 0.339″

Ceres is a dwarf planet in the main asteroid belt between the orbits of Mars and Jupiter. It was the first object identified in the asteroid belt, discovered on 1 January 1801 by Giuseppe Piazzi at Palermo Astronomical Observatory in Sicily, and announced as a new planet. Ceres was later classified as an asteroid, and then more recently as the only confirmed dwarf planet within the asteroid belt, and the largest without a moon. It is also the only recognized dwarf planet in the solar system whose orbit lies within that of Neptune. In the minor planet numbering system, its designation is 1 Ceres or (1) Ceres.

Ceres's diameter is about a quarter that of the Moon. Its small size means that even at its brightest it is too dim to be seen by the naked eye, except under extremely dark skies. Its apparent magnitude ranges from 6.7 to 9.3, peaking at opposition (when it is closest to Earth) once every 15- to 16-month synodic period. As a result, its surface features are barely visible even with the most powerful telescopes, and little was known about it until the robotic NASA spacecraft Dawn approached Ceres for its orbital mission in 2015.

Dawn found Ceres's surface to be a mixture of water, ice, and hydrated minerals such as carbonates and clay. Gravity data suggest Ceres to be partially differentiated into a muddy (ice–rock) mantle/core and a less dense, but stronger crust that is at most thirty percent ice by volume. Although Ceres likely has an internal ocean of liquid water, brines still flow through the outer mantle and reach the surface, allowing cryovolcanoes such as Ahuna Mons to form roughly every fifty million years. This makes Ceres the closest known cryovolcanically active body to the Sun. Ceres has an extremely tenuous and transient atmosphere of water vapour, vented from localised sources on its surface.