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51 Nemausa
Main-belt asteroid
Main-belt asteroid
| Field | Value |
|---|---|
| minorplanet | yes |
| background | #D6D6D6 |
| name | 51 Nemausa |
| image | 51 Nemausa VLT (2021), deconvolved.pdf |
| pronounced | |
| adjective | Nemausian |
| discoverer | J. Laurent |
| discovered | January 22, 1858 |
| discovery_site | Nîmes |
| mpc_name | (51) Nemausa |
| named_after | Nemausus |
| mp_category | Main belt |
| epoch | December 31, 2006 (JD 2454100.5) |
| semimajor | 2.365 AU (353.871 million km) |
| perihelion | 2.208 AU (330.360 million km) |
| aphelion | 2.523 AU (377.381 million km) |
| eccentricity | 0.066 |
| period | 3.64 a (1328.853 d) |
| inclination | 9.972° |
| asc_node | 176.168° |
| arg_peri | 2.820° |
| mean_anomaly | 316.668° |
| dimensions | 170×136 km{{cite web |
| title | Diameters |
| publisher | Astronomical Applications Department of the U.S. Naval Observatory |
| url | http://aa.usno.navy.mil/AsAtest/SecG/Diameters.txt |
| access-date | 2008-05-23 |
| url-status | dead |
| archive-url | https://web.archive.org/web/20110927084045/http://aa.usno.navy.mil/AsAtest/SecG/Diameters.txt |
| archive-date | 2011-09-27 |
| flattening | 0.23 |
| mean_diameter | |
| mass | |
| density | |
| rotation | 7.783 h |
| spectral_type | G |
| abs_magnitude | 7.74 |
| albedo | 0.09 (calculated) |
|access-date=2008-05-23 |url-status=dead |archive-url=https://web.archive.org/web/20110927084045/http://aa.usno.navy.mil/AsAtest/SecG/Diameters.txt |archive-date=2011-09-27
51 Nemausa is a large main-belt asteroid that was discovered on January 22, 1858, by Joseph Jean Pierre Laurent. Laurent made the discovery from the private observatory of Benjamin Valz in Nîmes, France. The house, at 32 rue Nationale in Nîmes, has a plaque commemorating the discovery. With Laurent's permission, Valz named the asteroid after the Celtic god Nemausus, the patron god and namesake of Nîmes during Roman times.
Based upon its spectrum, this is listed as a C-type asteroid in the Tholen classification taxonomy, and as a Cgh by Bus and Binzel (2002). This indicates a composition similar to carbonaceous chondrite meteorites. Absorption features in the spectrum indicate the presence of phyllosilicates. It may have a water content of about 14%.
The first stellar occultation was observed on August 17, 1979, from the Gissar and Alma-Ata observatories produced two chords which were used to estimate a diameter of 150 km for the asteroid. This is close to the present-day estimate of 147.9 km. Since then 51 Nemausa has been observed 20 times in stellar occultation.
Light curve inversion model DAMIT 1065 is a good match to a seven-chord occultation observed on 3 September 2016, from which an equivalent mean diameter of 146.4 km, and an equivalent Surface mean diameter of 150.3 km was obtained.
Lightcurve data suggests that it may have a small moon. Nemausa has been studied by radar.
|File:51Nemausa 20160903 (OccultationAndInversion).jpg |A light-curve Inversion model (DAMIT 1065) and a seven-chord occultation of 51 Nemausa |File:Observatoire de Marseille - Patrimoines 86209 676366.jpg |Chart dated 22 January 1858 |File:Observatoire de Marseille - Patrimoines 86209 676366 detail.jpg |Detail of handwritten legend at top ("J. Laurent")
Notes
References
References
- John Craig (1869) ''The Universal English Dictionary''
- P. Vernazza et al. (2021) VLT/SPHERE imaging survey of the largest main-belt asteroids: Final results and synthesis. ''Astronomy & Astrophysics'' 54, A56
- "51 Nemausa (A858 BA)".
0.093[http://www.psi.edu/pds/resource/albedo.html Asteroid Data Sets] {{webarchive. link. (2009-12-17)- Schmadel, Lutz D.. (2003). "Dictionary of Minor Planet Names". Springer Science & Business Media.
- "Asteroid Data Sets".
- [http://www.johnstonsarchive.net/astro/asteroidmoonsq.html Other reports of asteroid/TNO companions]
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