2 Pallas

Pallas (minor-planet designation: 2 Pallas) is the second asteroid to have been discovered, after Ceres. Like Ceres, it is believed to have a mineral composition similar to carbonaceous chondrite meteorites, though significantly less hydrated than Ceres. It is the third-largest asteroid in the Solar System by both volume and mass, and is a likely remnant protoplanet. It is 79% the mass of Vesta and 22% the mass of Ceres, constituting an estimated 7% of the mass of the asteroid belt. Its estimated volume is equivalent to a sphere 507 to 515 kilometers (315 to 320 mi) in diameter, 90–95% the volume of Vesta.

2 Pallas
VLT-SPHERE image of Pallas
Discovery
Discovered byHeinrich Wilhelm Olbers
Discovery date28 March 1802
Designations
MPC designation
(2) Pallas
Pronunciation/ˈpæləs/
Named after
Pallas Athena
Minor planet category
Asteroid belt (central)
Pallas family
AdjectivesPalladian (/pæˈldiən/)
Symbol (historically astronomical, now astrological)
Orbital characteristics
Epoch 13 September 2023
(JD 2453300.5)
Uncertainty parameter 0
Observation arc219 yr
Aphelion3.41 AU (510 million km)
Perihelion2.13 AU (319 million km)
Semi-major axis
2.77 AU (414 million km)
Eccentricity0.2302
Orbital period (sidereal)
4.611 yr (1,684.0 d)
Mean anomaly
40.6
Mean motion
0° 12m 46.8s / day
Inclination34.93°
(34.43° to invariable plane)
Longitude of ascending node
172.9°
7 March 2023
310.9°
Earth MOID1.2 AU (180 million km)
Proper orbital elements
Proper semi-major axis
2.7709176 AU
Proper eccentricity
0.2812580
Proper inclination
33.1988686°
Proper mean motion
78.041654 deg / yr
Proper orbital period
4.61292 yr
(1684.869 d)
Precession of perihelion
−1.335344 arcsec / yr
Precession of the ascending node
−46.393342 arcsec / yr
Physical characteristics
Dimensionsc/a = 0.79±0.03
568 ±12 km × 532 ±12 km × 448 ±12 km
550 km × 516 km × 476 km
Mean diameter
511±4
513±6 km
512±6 km
Surface area
(8.3±0.2)×105 km2 (2020)
Volume(7.06±0.3)×107 km3 (2020)
Mass(2.04±0.03)×1020 kg average est.
(2.01±0.13)×1020 kg
Mean density
2.92±0.08 g/cm3
2.89±0.08 g/cm3
2.57±0.19 g/cm3
Equatorial surface gravity
≈0.21 m/s2 (average)
0.022 g
Equatorial escape velocity
324 m/s
Synodic rotation period
7.8132 h
Equatorial rotation velocity
65 m/s
84°±
0.155
0.159
B
6.49 to 10.65
4.13
0.629″ to 0.171″

During the planetary formation era of the Solar System, objects grew in size through an accretion process to approximately the size of Pallas. Most of these protoplanets were incorporated into the growth of larger bodies, which became the planets, whereas others were ejected by the planets or destroyed in collisions with each other. Pallas, Vesta and Ceres appear to be the only intact bodies from this early stage of planetary formation to survive within the orbit of Neptune.

When Pallas was discovered by the German astronomer Heinrich Wilhelm Matthäus Olbers on 28 March 1802, it was considered to be a planet, as were other asteroids in the early 19th century. The discovery of many more asteroids after 1845 eventually led to the separate listing of "minor" planets from "major" planets, and the realization in the 1950s that such small bodies did not form in the same way as (other) planets led to the gradual abandonment of the term "minor planet" in favor of "asteroid" (or, for larger bodies such as Pallas, "planetoid").

With an orbital inclination of 34.8°, Pallas's orbit is unusually highly inclined to the plane of the asteroid belt, making Pallas relatively inaccessible to spacecraft, and its orbital eccentricity is nearly as large as that of Pluto.

The high inclination of the orbit of Pallas results in the possibility of close conjunctions to stars that other solar objects always pass at great angular distance. This resulted in Pallas passing Sirius on 9 October 2022, only 8.5 arcminutes southwards, while no planet can get closer than 30 degrees to Sirius.

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