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4257 Ubasti

From Wikipedia, the free encyclopedia
Near-Earth asteroid

4257 Ubasti
Discovery[1]
Discovered byJ. E. Mueller
Discovery sitePalomar Obs.
Discovery date23 August 1987
Designations
(4257) Ubasti
Named after
Bastet[2]
(Egyptian goddess of cats)
1987 QA
NEO · Apollo[1][3]
Mars-crosser
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc29.02 yr (10,600 days)
Aphelion2.4183AU
Perihelion0.8759 AU
1.6471 AU
Eccentricity0.4682
2.11yr (772 days)
28.670°
0° 27m 58.32s / day
Inclination40.716°
169.22°
278.92°
Earth MOID0.1714 AU · 66.8LD
Physical characteristics
Dimensions1.30±0.09 km[4]
1.96 km(calculated)[5]
0.20(assumed)[5]
0.376±0.053[4]
S[5]
15.9[1][5] · 16.20[4]

4257 Ubasti, provisional designation1987 QA, is a stonyasteroid, classified asnear-Earth object of theApollo group and asMars-crosser, approximately 1.5 kilometers in diameter. It was discovered by American astronomerJean Mueller at thePalomar Observatory in California on 23 August 1987.[3] The asteroid was named forBastet – also known as Baast, Ubaste or Ubasti – the Egyptian goddess of cats.[2]

Orbit and classification

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Ubasti orbits the Sun at a distance of 0.9–2.4 AU once every 2 years and 1 month (772 days). Its orbit has aneccentricity of 0.47 and aninclination of 41° with respect to theecliptic.[1] Due to its high eccentricity,Ubasti is also aMars-crossing asteroid. The body'sobservation arc begins with its official discovery observation, as noprecoveries were taken and no prior identification had been made.[3]

Close approaches

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As anear-Earth object,Ubasti has a low Earthminimum orbital intersection distance of 0.1714 AU (25,600,000 km), which corresponds to 66.8lunar distances (LD). This distance, however, is too large to make it apotentially hazardous asteroid (0.05 AU; less than 20 LD).[1]

Physical characteristics

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Ubasti is an assumed stonyS-type asteroid.[5]

Rotation period

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As of 2017, no rotationallightcurve ofUbasti has been obtained and itsrotation period remains unknown.[5] However, theLowell Observatory Near-Earth Asteroid Photometric Survey has measured the body's brightness variation caused by its rotation, which gave a maximum of 0.36magnitude. This indicates that the body has a somewhat non-spherical shape.[6]

Diameter and albedo

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According to the survey carried out by the JapaneseAkari satellite,Ubasti measures 1.30 kilometers in diameter and its surface has analbedo of 0.376,[4] while theCollaborative Asteroid Lightcurve Link assumes a standard albedo for stony asteroids of 0.20 and calculates a diameter of 1.96 kilometers based on anabsolute magnitude of 15.9.[5]

Naming

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Thisminor planet was named after Egyptian goddessesBastet, who was originally the goddess of warfare, equated with the lioness war goddess, but later transformed into a major protector deity represented as a cat.[2] The official naming citation was published by theMinor Planet Center on 21 November 1991 (M.P.C. 19336).[7] The discoverer dedicated this asteroid to her beloved companion, Pepper Cat (1974–1991).[2]

References

[edit]
  1. ^abcdef"JPL Small-Body Database Browser: 4257 Ubasti (1987 QA)" (2016-08-30 last obs.).Jet Propulsion Laboratory. Retrieved15 September 2017.
  2. ^abcdSchmadel, Lutz D. (2007). "(4257) Ubasti".Dictionary of Minor Planet Names – (4257) Ubasti.Springer Berlin Heidelberg. p. 365.doi:10.1007/978-3-540-29925-7_4219.ISBN 978-3-540-00238-3.
  3. ^abc"4257 Ubasti (1987 QA)".Minor Planet Center. Retrieved15 September 2017.
  4. ^abcdUsui, Fumihiko; Kuroda, Daisuke; Müller, Thomas G.; Hasegawa, Sunao; Ishiguro, Masateru; Ootsubo, Takafumi; et al. (October 2011). "Asteroid Catalog Using Akari: AKARI/IRC Mid-Infrared Asteroid Survey".Publications of the Astronomical Society of Japan.63 (5):1117–1138.Bibcode:2011PASJ...63.1117U.doi:10.1093/pasj/63.5.1117. (online,AcuA catalog p. 153)
  5. ^abcdefg"LCDB Data for (4257) Ubasti". Asteroid Lightcurve Database (LCDB). Retrieved15 September 2017.
  6. ^Skiff, Brian A.; Bowell, Edward; Koehn, Bruce W.; Sanborn, Jason J.; McLelland, Kyle P.; Warner, Brian D. (July 2012)."Lowell Observatory Near-Earth Asteroid Photometric Survey (NEAPS) - 2008 May through 2008 December".The Minor Planet Bulletin.39 (3):111–130.Bibcode:2012MPBu...39..111S.ISSN 1052-8091. Retrieved15 September 2017.
  7. ^"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved15 September 2017.

External links

[edit]
Minor planets
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Authority control databasesEdit this at Wikidata
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