Astronomy:10979 Fristephenson
| Discovery[1] | |
|---|---|
| Discovered by | C. J. van Houten I. van Houten-G. T. Gehrels |
| Discovery site | Palomar Obs. |
| Discovery date | 29 September 1973 |
| Designations | |
| (10979) Fristephenson | |
| Named after | Francis Richard Stephenson[1] (British historian of astronomy) |
| 4171 T-2 · 4386 T-3 | |
| Minor planet category | main-belt[1][2] · (inner) Sulamitis[3] |
| Orbital characteristics[2] | |
| Epoch 23 March 2018 (JD 2458200.5) | |
| Uncertainty parameter 0 | |
| Observation arc | 44.52 yr (16,260 d) |
| |{{{apsis}}}|helion}} | 2.6597 AU |
| |{{{apsis}}}|helion}} | 2.2555 AU |
| 2.4576 AU | |
| Eccentricity | 0.0822 |
| Orbital period | 3.85 yr (1,407 d) |
| Mean anomaly | 292.96° |
| Mean motion | 0° 15m 20.88s / day |
| Inclination | 5.5613° |
| Longitude of ascending node | 138.32° |
| 122.19° | |
| Physical characteristics | |
| Mean diameter | 5.327±0.069 km[4] |
| Geometric albedo | 0.057±0.009[4] |
| C (SDSS-MOC)[5] | |
| Absolute magnitude (H) | 15.1[2] |
10979 Fristephenson (provisional designation 4171 T-2) is a carbonaceous Sulamitis asteroid from the inner regions of the asteroid belt, approximately 5 kilometers (3.1 miles) in diameter. It was discovered during the Palomar–Leiden Trojan survey on 29 September 1973, by Ingrid and Cornelis van Houten at Leiden, and Tom Gehrels at Palomar Observatory in California, United States. The dark C-type asteroid was named for British historian of astronomy Francis Richard Stephenson.[1]
Orbit and classification
Fristephenson is a member of the Sulamitis family (408),[3] a small family of 300 known carbonaceous asteroids named after 752 Sulamitis.[6] It orbits the Sun in the inner main-belt at a distance of 2.3–2.7 AU once every 3 years and 10 months (1,407 days; semi-major axis of 2.46 AU). Its orbit has an eccentricity of 0.08 and an inclination of 6° with respect to the ecliptic.[2] The body's observation arc begins at Palomar on 19 September 1973, ten days after its official discovery observation.[1]
Palomar–Leiden Trojan survey
Physical characteristics
Fristephenson has an absolute magnitude of 15.1.[2] Based on the Moving Object Catalog (MOC) of the Sloan Digital Sky Survey, the asteroid has a spectral type of a carbonaceous C-type asteroid,[5] which agrees with its classification into the Sulamitis family,[6] as well as with its low Geometric albedo measured by the Wide-field Infrared Survey Explorer.[2] As of 2018, no rotational lightcurve has been obtained from photometric observations. The body's rotation period, pole and shape remain unknown.[2]
Diameter and albedo
According to the survey carried out by the NEOWISE mission of NASA's WISE telescope, Fristephenson measures 5.327 kilometers in diameter and its surface has an albedo of 0.057.[4]
Naming
This minor planet was named after Francis Richard Stephenson (born 1941), a British historian of astronomy at Durham University. The official naming citation was published by the Minor Planet Center on 26 November 2004 (M.P.C. 53174).[7]
References
- ↑ 1.0 1.1 1.2 1.3 1.4 "10979 Fristephenson (4171 T-2)". Minor Planet Center. https://www.minorplanetcenter.net/db_search/show_object?object_id=10979.
- ↑ 2.0 2.1 2.2 2.3 2.4 2.5 2.6 "JPL Small-Body Database Browser: 10979 Fristephenson (4171 T-2)". Jet Propulsion Laboratory. https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=2010979.
- ↑ 3.0 3.1 "Asteroid 10979 Fristephenson – Nesvorny HCM Asteroid Families V3.0". Small Bodies Data Ferret. https://sbntools.psi.edu/ferret/SimpleSearch/results.action?targetName=10979+Fristephenson#Asteroid%2010979%20FristephensonEAR-A-VARGBDET-5-NESVORNYFAM-V3.0.
- ↑ 4.0 4.1 4.2 Masiero, Joseph R.; Mainzer, A. K.; Grav, T.; Bauer, J. M.; Cutri, R. M.; Dailey, J. et al. (November 2011). "Main Belt Asteroids with WISE/NEOWISE. I. Preliminary Albedos and Diameters". The Astrophysical Journal 741 (2): 20. doi:10.1088/0004-637X/741/2/68. Bibcode: 2011ApJ...741...68M.
- ↑ 5.0 5.1 Carvano, J. M.; Hasselmann, P. H.; Lazzaro, D.; Mothé-Diniz, T. (February 2010). "SDSS-based taxonomic classification and orbital distribution of main belt asteroids". Astronomy and Astrophysics 510: 12. doi:10.1051/0004-6361/200913322. Bibcode: 2010A&A...510A..43C. https://sbnarchive.psi.edu/pds3/non_mission/EAR_A_I0035_5_SDSSTAX_V1_1/data/sdsstax_ast_table.tab. Retrieved 30 October 2019. (PDS data set)
- ↑ 6.0 6.1 Nesvorný, D.; Broz, M.; Carruba, V. (December 2014). "Identification and Dynamical Properties of Asteroid Families". Asteroids IV. pp. 297–321. doi:10.2458/azu_uapress_9780816532131-ch016. ISBN 9780816532131. Bibcode: 2015aste.book..297N.
- ↑ "MPC/MPO/MPS Archive". Minor Planet Center. https://www.minorplanetcenter.net/iau/ECS/MPCArchive/MPCArchive_TBL.html.
<ref> tag with name "MPC-discoverers" defined in <references> is not used in prior text.External links
- Asteroid Lightcurve Database (LCDB), query form (info )
- Dictionary of Minor Planet Names, Google books
- Discovery Circumstances: Numbered Minor Planets (10001)-(15000) – Minor Planet Center
- 10979 Fristephenson at AstDyS-2, Asteroids—Dynamic Site
- 10979 Fristephenson at the JPL Small-Body Database
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