Movatterモバイル変換


[0]ホーム

URL:


Jump to content
WikipediaThe Free Encyclopedia
Search

268 Adorea

From Wikipedia, the free encyclopedia
Main-belt asteroid
"Adorea" redirects here. For the insect genus, seeAdorea (beetle).

268 Adorea
Orbital diagram
Discovery
Discovered byAlphonse Borrelly
Discovery date8 June 1887
Designations
(268) Adorea
Pronunciation/əˈdɔːriə/
Named after
adorea liba (spelt cakes)
A887 LA
Main belt (Themis)
AdjectivesAdorean/əˈdɔːriən/
Orbital characteristics[1]
Epoch 31 July 2016 (JD 2457600.5)
Uncertainty parameter 0
Observation arc39,920 d (109.3 yr)
Aphelion3.515 AU (525.8 Gm)
Perihelion2.668 AU (399.2 Gm)
3.092 AU (462.5 Gm)
Eccentricity0.13689
5.44 yr (1,985.5 d)
302.257°
0° 10m 52.748s / day
Inclination2.44010°
120.914°
69.5742°
Physical characteristics
144.585±0.892 km[1]
139.57±3.31 km[2]
Mass(2.228 ± 0.919/0.718)×1018 kg[2]
1.565 ± 0.645/0.505 g/cm3[2]
7.80 h (0.325 d)
0.041±0.007[1]
FC
8.67[1]

268 Adorea is a very largemain belt asteroid, about 140 km (87 mi) in width. It was discovered byAlphonse Borrelly on 8 June 1887 inMarseille. This asteroid is a member of theThemis family[3] and is classified as a primitivecarbonaceousF-type/C-type asteroid. It is orbiting theSun at a distance of3.09 AU with anorbital eccentricity (ovalness) of 0.14 and aperiod of 5.44 yr. Theorbital plane is tilted at an angle of 2.44° to theplane of the ecliptic.[1]

From 23 February until 2 March 2006,photometric measurements were taken of the asteroid. These were used to produce alight curve showing arotation period of7.80±0.02 h with a brightness variation of0.16±0.03 inmagnitude. This result is consistent with some, but not all previous results. Some studies had suggested a longer rotation period of15.959 h; double the time measured. However, the new data is inconsistent with the longer period.[4]

In May 1979, 268 Adorea was positioned in proximity of the galaxyNGC 4517 and as a bright new light source it was identified as a potentialsupernova. However, the light was missing from a second photographic plate taken ten days later, and the source was soon identified as the asteroid.[5]

The name refers toadorea liba, theLatin name forspelt cakes produced from meal and salt offered by the Romans as a sacrifice; the name was controversial among astronomers, as all previous asteroids had been named for humans or mythological figures.[6][7]

References

[edit]
  1. ^abcde"268 Adorea".JPL Small-Body Database.NASA/Jet Propulsion Laboratory. Retrieved11 May 2016.
  2. ^abcFienga, 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.
  3. ^Florczak, M.; et al. (February 1999)."A spectroscopic study of the THEMIS family".Astronomy and Astrophysics Supplement.134 (3):463–471.Bibcode:1999A&AS..134..463F.doi:10.1051/aas:1999150.
  4. ^Stephens, Robert D. (December 2006). "Asteroid lightcurve photometry from Santana and GMARS observatories - winter and spring 2006".Bulletin of the Minor Planets Section of the Association of Lunar and Planetary Observers.33 (4):100–101.Bibcode:2006MPBu...33..100S.
  5. ^West, R. (September 1979). "The Supernova that was not - 268 Adorea".The Messenger (18): 14.Bibcode:1979Msngr..18...14W.
  6. ^Schmadel, Lutz (5 August 2003).Dictionary of Minor Planet Names. Springer Science & Business Media.ISBN 9783540002383 – via Google Books.
  7. ^"268 Adorea".markandrewholmes.com.

External links

[edit]
Minor planets
Asteroid
Distant minor planet
Comets
Other
Authority control databasesEdit this at Wikidata
Retrieved from "https://en.wikipedia.org/w/index.php?title=268_Adorea&oldid=1285877331"
Categories:
Hidden categories:

[8]ページ先頭

©2009-2025 Movatter.jp