10979 Fristephenson
Discovery[1]
Discovered byC. J. van Houten
I. van Houten-G.
T. Gehrels
Discovery sitePalomar Obs.
Discovery date29 September 1973
Designations
(10979) Fristephenson
Named after
Francis Richard Stephenson[1]
(British historian of astronomy)
4171 T-2 · 4386 T-3
main-belt[1][2] · (inner)
Sulamitis[3]
Orbital characteristics[2]
Epoch 23 March 2018 (JD 2458200.5)
Uncertainty parameter 0
Observation arc44.52 yr (16,260 d)
Aphelion2.6597 AU
Perihelion2.2555 AU
2.4576 AU
Eccentricity0.0822
3.85 yr (1,407 d)
292.96°
0° 15m 20.88s / day
Inclination5.5613°
138.32°
122.19°
Physical characteristics
Mean diameter
5.327±0.069 km[4]
0.057±0.009[4]
C (SDSS-MOC)[5]
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

    The survey designation "T-2" stands for the second Palomar–Leiden Trojan survey, named after the fruitful collaboration of the Palomar and Leiden Observatory during the 1960s and 1970s. Gehrels used Palomar's Samuel Oschin telescope (also known as the 48-inch Schmidt Telescope), and shipped the photographic plates to Ingrid and Cornelis van Houten at Leiden Observatory where astrometry was carried out. The trio are credited with the discovery of several thousand asteroid discoveries.[7]

    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).[8]

    References

    1. 1 2 3 4 5 "10979 Fristephenson (4171 T-2)". Minor Planet Center. Retrieved 1 May 2018.
    2. 1 2 3 4 5 6 7 "JPL Small-Body Database Browser: 10979 Fristephenson (4171 T-2)" (2018-03-27 last obs.). Jet Propulsion Laboratory. Retrieved 1 May 2018.
    3. 1 2 "Asteroid 10979 Fristephenson – Nesvorny HCM Asteroid Families V3.0". Small Bodies Data Ferret. Retrieved 27 October 2019.
    4. 1 2 3 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. arXiv:1109.4096. Bibcode:2011ApJ...741...68M. doi:10.1088/0004-637X/741/2/68.
    5. 1 2 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. Bibcode:2010A&A...510A..43C. doi:10.1051/0004-6361/200913322. Retrieved 30 October 2019. (PDS data set)
    6. 1 2 Nesvorný, D.; Broz, M.; Carruba, V. (December 2014). "Identification and Dynamical Properties of Asteroid Families". Asteroids IV. pp. 297–321. arXiv:1502.01628. Bibcode:2015aste.book..297N. doi:10.2458/azu_uapress_9780816532131-ch016. ISBN 9780816532131.
    7. ↑ "Minor Planet Discoverers". Minor Planet Center. 2018. Retrieved 1 May 2018.
    8. ↑ "MPC/MPO/MPS Archive". Minor Planet Center. Retrieved 1 May 2018.
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