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4401 Aditi
Eccentric, stony asteroid
Eccentric, stony asteroid
| Field | Value | |||
|---|---|---|---|---|
| minorplanet | yes | |||
| name | 4401 Aditi | |||
| background | #FFC2E0 | |||
| discovery_ref | ||||
| discovered | 14 October 1985 | |||
| discoverer | C. Shoemaker | |||
| discovery_site | Palomar Obs. | |||
| mpc_name | (4401) Aditi | |||
| alt_names | 1985 TB | |||
| named_after | Aditi (Hindu goddess) | |||
| mp_category | {{Hlist | |||
| Amor<ref name | "jpldata" / | |||
| orbit_ref | ||||
| epoch | 4 September 2017 (JD 2458000.5) | |||
| uncertainty | 0 | |||
| observation_arc | 29.57 yr (10,800 days) | |||
| aphelion | 4.0367 AU | |||
| perihelion | 1.1228 AU | |||
| semimajor | 2.5797 AU | |||
| eccentricity | 0.5648 | |||
| period | 4.14 yr (1,513 days) | |||
| mean_anomaly | 235.58° | |||
| mean_motion | / day | |||
| inclination | 26.650° | |||
| asc_node | 22.902° | |||
| arg_peri | 68.144° | |||
| moid | 0.3302 AU (128.6 LD) | |||
| dimensions | {{Ubl | |||
| {{val | 1.801 | 0.535 | u | km}} |
| 1.88 km <ref name | "lcdb" / | |||
| rotation | {{Ubl | |||
| {{val | 6.670 | 0.005 | ul | h}} |
| {{val | 6.6780 | 0.0005 | u | h}} |
| {{val | 6.683 | 0.005 | u | h}} |
| {{val | 19.2 | 0.5 | u | h}} |
| albedo | {{Ubl | |||
| 0.20 <ref name | "lcdb" / | |||
| <ref name | "Mainzer-2012" / | |||
| spectral_type | S | |||
| abs_magnitude | {{Hlist | |||
| 15.50<ref name | "Mainzer-2012" / | |||
| 16.0<ref name | "jpldata" / |
| NEO | Amor | | 1.88 km (calculated) | | | | | 0.20 (assumed) | | 15.50 | 16.0
4401 Aditi (provisional designation ****) is an eccentric, stony asteroid, classified as a near-Earth object and Amor asteroid, approximately 1.8 kilometers in diameter. It was discovered on 14 October 1985 by American astronomer Carolyn Shoemaker at Palomar Observatory in California, and later named after the Hindu goddess Aditi.
Classification and orbit
Aditi orbits the Sun at a distance of 1.1–4.0 AU once every 4 years and 2 months (1,513 days). Its orbit has an eccentricity of 0.56 and an inclination of 27° with respect to the ecliptic. The asteroid's observation arc begins with its discovery, as no precoveries were taken and no identifications were made before 1985.
With an Earth minimum orbit intersection distance, MOID, of 0.3302 AU, or 128.6 lunar distances, it 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.
Physical characteristics
Lightcurves
Two rotational lightcurves of Aditi were obtained from photometric observations by American astronomer Brian Warner at his Palmer Divide Observatory, Colorado, in August 2014 and March 2015, respectively. The first lightcurve rendered a period of hours with a brightness variation of 0.64 (), while the second one gave a period of hours with an amplitude of 0.29 magnitude ().
Additional lightcurves were obtained by Benishek () and Manzini ().
Diameter and albedo
According to the survey carried out by NASA's space-based Wide-field Infrared Survey Explorer with its subsequent NEOWISE mission, Aditi has a high albedo of 0.34 with a corresponding diameter of 1.80 kilometers.
The Collaborative Asteroid Lightcurve Link assumes a standard albedo for stony S-type asteroids of 0.20 and calculates a slightly larger diameter of 1.88 kilometers, as the lower the body's albedo (reflectivity), the higher its diameter, at a constant absolute magnitude (brightness).
Naming
This minor planet is named after the Hindu goddess Aditi, celestial mother of every existing form and being. 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. The official naming citation was published on 30 January 1991 (M.P.C. ).
Notes
References
- 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
This article was imported from Wikipedia and is available under the Creative Commons Attribution-ShareAlike 4.0 License. Content has been adapted to SurfDoc format. Original contributors can be found on the article history page.
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