4401 Aditi
| Discovery [1] | |
|---|---|
| Discovered by | C. Shoemaker |
| Discovery site | Palomar Obs. |
| Discovery date | 14 October 1985 |
| Designations | |
| 4401 Aditi | |
Named after | Aditi (Hindu goddess)[2] |
| 1985 TB | |
| Amor · NEO | |
| Orbital characteristics [1] | |
| Epoch 13 January 2016 (JD 2457400.5) | |
| Uncertainty parameter 0 | |
| Observation arc | 29.57 yr (10,800 days) |
| Aphelion | 4.0369 AU |
| Perihelion | 1.1222 AU |
| 2.5795 AU | |
| Eccentricity | 0.5649 |
| 4.14 yr (1,513 days) | |
| 92.769° | |
| Inclination | 26.651° |
| 22.910° | |
| 68.159° | |
| Earth MOID | 0.3289 AU |
| Physical characteristics | |
| Dimensions | 1.801±0.535 km[3] 1.88 km (calculated)[4] |
| 6.670±0.005 h[5] 6.683±0.005 h[6] 6.6780±0.0005 h[a] 19.2±0.5 h[7] | |
| 0.343±0.204[3] 0.20 (assumed)[4] | |
| S [4] | |
| 16.0[1][4] 15.50[3] | |
4401 Aditi, provisional designation 1985 TB, is an eccentric, stony asteroid, classified as near-Earth object and Amor asteroid, about 1.8 kilometers in diameter. It was discovered by American female astronomer Carolyn Shoemaker at the U.S. Palomar Observatory, California, on 14 October 1985.[8]
The S-type asteroid orbits the Sun at a distance of 1.1–4.0 AU once every 4 years and 2 months (1,513 days). Its orbit shows a typically high eccentricity of 0.56 and an inclination of 27 degrees from the plane of the ecliptic. With an Earth minimum orbit intersection distance (MOID) of 0.33 AU (49,000,000 km), the asteroid never approaches Earth close enough to be classified as a potentially hazardous object, for which an upper MOID-limit of 0.05 AU is defined.[1]
In 2014 and 2015, two photometric light-curve analysis at the U.S Palmer Divide Observatory (PDO) in Colorado rendered a rotation period of 6.670±0.005 hours with a brightness amplitude of 0.29 in magnitude (best result, U=3).[5][6] Other light-curve observations were performed by Benishek[a] and Manzini.[7]
According to the survey carried out by NASA's Wide-field Infrared Survey Explorer with its subsequent NEOWISE mission, the body has a high albedo of 0.34 with a corresponding diameter of 1.8 kilometers.[3] The Collaborative Asteroid Lightcurve Link (CALL) assumes a standard albedo of 0.20 and calculates a slightly larger diameter of 1.9 kilometers, as the lower the body's albedo (reflectivity), the higher its diameter, for a given absolute magnitude (brightness).[4]
The minor planet is named after Aditi, the Hindu goddess of the sky and the air. She was the mother of the thirty-three gods, including the Vasus, the Rudras, and the Ādityas, the twelve zodiacal spirits. She is described in Vedic literature as the gods of the heavenly light.[2]
References
- ^ a b Benishek (2014) web: rotation period 19.2±0.5 hours with a brightness amplitude of 0.55 mag. No LCDB Quality Code available. Summary figures at Collaborative Asteroid Lightcurve Link (CALL) for (4401) Aditi
- ^ a b c d "JPL Small-Body Database Browser: 4401 Aditi (1985 TB)" (2015-05-10 last obs.). Jet Propulsion Laboratory. Retrieved February 2016.
{{cite web}}: Check date values in:|accessdate=(help) - ^ a b Schmadel, Lutz D. (2007). Dictionary of Minor Planet Names – (4401) Aditi. Springer Berlin Heidelberg. p. 378. ISBN 978-3-540-00238-3. Retrieved February 2016.
{{cite book}}: Check date values in:|accessdate=(help) - ^ a b c d Mainzer, A.; Grav, T.; Masiero, J.; Bauer, J.; Cutri, R. M.; McMillan, R. S.; et al. (November 2012). "Physical Parameters of Asteroids Estimated from the WISE 3-Band Data and NEOWISE Post-Cryogenic Survey". The Astrophysical Journal Letters. 760 (1): 6. arXiv:1210.0502. Bibcode:2012ApJ...760L..12M. doi:10.1088/2041-8205/760/1/L12. Retrieved February 2016.
{{cite journal}}: Check date values in:|access-date=(help) - ^ a b c d e "LCDB Data for (4401) Aditi". Asteroid Lightcurve Database (LCDB). Retrieved February 2016.
{{cite web}}: Check date values in:|accessdate=(help) - ^ a b Warner, Brian D. (July 2015). "Near-Earth Asteroid Lightcurve Analysis at CS3-Palmer Divide Station: 2015 January - March". The Minor Planet Bulletin. 42 (3): 172–183. Bibcode:2015MPBu...42..172W. ISSN 1052-8091. Retrieved February 2016.
{{cite journal}}: Check date values in:|access-date=(help) - ^ a b Warner, Brian D. (January 2015). "Near-Earth Asteroid Lightcurve Analysis at CS3-Palmer Divide Station: 2014 June-October". The Minor Planet Bulletin. 42 (1): 41–53. Bibcode:2015MPBu...42...41W. ISSN 1052-8091. Retrieved February 2016.
{{cite journal}}: Check date values in:|access-date=(help) - ^ a b Behrend, Raoul. "Asteroids and comets rotation curves – (4401) Aditi". Geneva Observatory. Retrieved February 2016.
{{cite web}}: Check date values in:|accessdate=(help) - ^ "4401 Aditi (1985 TB)". Minor Planet Center. Retrieved February 2016.
{{cite web}}: Check date values in:|accessdate=(help)
External links
- NEODyS-2 for (4401) Aditi
- earn.dlr.de/nea for (4401) Aditi
- Asteroid Lightcurve Database (LCDB), query form (info)
- Dictionary of Minor Planet Names, Google books
- Asteroids and comets rotation curves, CdR – Observatoire de Genève, Raoul Behrend
- Discovery Circumstances: Numbered Minor Planets (1)-(5000) – Minor Planet Center
- 4401 Aditi at the JPL Small-Body Database
- The Palmer Divide Observatory: Tour given by Brian Warner on YouTube (time 4:03 min.)
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