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203 Pompeja

From Wikipedia, the free encyclopedia
Main-belt asteroid

203 Pompeja
Orbital diagram
Discovery
Discovered byC. H. F. Peters
Discovery date25 September 1879
Designations
(203) Pompeja
Pronunciation/pɒmˈpə/[1]
Named after
Pompeii
A879 SA, 1895 EA
Main belt
Orbital characteristics[2]
Epoch 31 July 2016 (JD 2457600.5)
Uncertainty parameter 0
Observation arc136.43 yr (49,832 d)
Aphelion2.897 AU (433.4 Gm)
Perihelion2.577 AU (385.5 Gm)
2.737 AU (409.4 Gm)
Eccentricity0.058490
4.53 yr (1,653.6 d)
18.01 km/s
47.6383°
0° 13m 3.72s / day
Inclination3.1780°
347.916°
57.060°
Physical characteristics
124.592±1.079 km[2]
Mass(1.251 ± 0.640/0.401)×1018 kg[3]
1.626 ± 0.831/0.521 g/cm3[3][a]
24.052 h (1.0022 d)[4][2]
0.036±0.006[2]
DCX:
8.97[2]

203 Pompeja is a fairly largemain-beltasteroid. It was discovered byC. H. F. Peters on September 25, 1879, inClinton, New York, and named afterPompeii, theRoman town destroyed involcanic eruption inAD 79. This asteroid is orbiting theSun at a distance of2.74 AU with aneccentricity (ovalness) of 0.06 and aperiod of 4.53 yr. Theorbital plane is tilted at an angle of 3.2° to theplane of the ecliptic.[2]

Based uponphotometric observations taken during 2011, it has a synodicrotation period of 24.052 ± 0.001 h, with a peak-to-peak amplitude of 0.10 ± 0.01 inmagnitude. Because the rotation period nearly matches that of the Earth, it required coordinated observations from multiple observatories at widely spaced latitudes to produce a completelight curve.[4] As discovered in 2021, Pompeja alongside the main-belt asteroid269 Justitia have very red colors due totholins on its surface, similar totrans-Neptunian objects. These asteroids are therefore thought to have formed in the outer Solar System despite their current orbits within the asteroid belt.[5]

Notes

[edit]
  1. ^Assuming a diameter of 113.68 ± 6.55 km.

References

[edit]
  1. ^'Pompeia' in Noah Webster (1884)A Practical Dictionary of the English Language
  2. ^abcdef"203 Pompeja".JPL Small-Body Database.NASA/Jet Propulsion Laboratory. Retrieved12 May 2016.
  3. ^abFienga, A.; Avdellidou, C.; Hanuš, J. (February 2020)."Asteroid masses obtained with INPOP planetary ephemerides".Monthly Notices of the Royal Astronomical Society.492 (1).doi:10.1093/mnras/stz3407.
  4. ^abPilcher, Frederick; et al. (July 2012), "Rotation Period Determination for 203 Pompeja - Another Triumph of Global Collaboration",The Minor Planet Bulletin,39 (3): 99,Bibcode:2012MPBu...39...99P
  5. ^Hasegawa, Sunao; Marsset, Michaël; Demeo, Francesca E.; Bus, Schelte J.; Geem, Jooyeon; Ishiguro, Masateru; Im, Myungshin; Kuroda, Daisuke; Vernazza, Pierre (2021), "Discovery of two TNO-like bodies in the asteroid belt",The Astrophysical Journal Letters,916 (1): L6,arXiv:2106.14991,Bibcode:2021ApJ...916L...6H,doi:10.3847/2041-8213/ac0f05,S2CID 235669878

External links

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