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107 Camilla

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Asteroid with 2 moons article August 2026 Replace shape model image with newer one May 2024 yes 107 Camilla #D6D6D6 107Camilla (Lightcurve Inversion).png Lightcurve-based 3-D model of Camilla line-height: 1.3em; 17 November 1868 N. R. Pogson Madras Obs. (107) Camilla A868 WA, 1893 QA1938 OG, 1949 HD 1 k ə ˈ m ɪ l əNoah Webster (1884) A Practical Dictionary of the English Language Camillian or Camillean, k ə ˈ m ɪ l i ə n Camilla (Roman mythology) main-belt(outer)SylviaCybele 23 March 2018 (JD 2458200.5) 0 149.17 yr (54,485 d) 3.7202 AU 3.2622 AU 3.4912 AU 0.0656 6.52 yr (2,383 d) 265.91° 0.1511 ms / day 10.001° 172.61° 306.77° 2 285 x 205 x 170 km344 x 246 x 205 km 254 12 km200.37 3.51 km210.370 8.326 km222.62 17.1 km241.6 35.0 km243.3 12.4 km 11.2 0.1 18 kg 1.28 .04 g/cm31.40 0.30 g/cm3 4.844 hLCDB-Pietschnig-2011 0.043 0.0120.045 0.0190.0525 0.0090.059 0.0120.065 0.003 X (SMASS)C (Tholen)P (WISE)B–V 0.705U–B 0.298 11.53 7.087.1 0.02 thumb|A lightcurve model of the asteroid on the top and an image of the asteroid on the bottom, with at least one of its moons barely visible in the first few images 107 Camilla is one of the largest asteroids from the outermost edge of the asteroid belt, approximately 250 km mi off us in diameter. It is a member of the Sylvia family and located within the Cybele group. It was discovered on 17 November 1868, by English astronomer Norman Pogson at Madras Observatory, India, and named after Camilla, Queen of the Volsci in Roman mythology. The X-type asteroid is a rare triple asteroid with two minor-planet moons discovered in 2001 and 2016, respectively. It is elongated in shape and has a short rotation period of 4.8 hours. Physical characteristics Camilla has a very dark surface and primitive carbonaceous composition. A large number of rotational lightcurves of have been obtained from photometric observations since the 1980s. Best rated results gave a short rotation period of 4.844 hours with a brightness amplitude between 0.32 and 0.53 magnitude.LCDB-Pietschnig-2011 Lightcurve analysis indicates that Camilla's pole most likely points towards ecliptic coordinates (β, λ) = (+51°, 72°) with a 10° uncertainty, which gives it an axial tilt of 29°. Follow-up modeling of photometric data gave similar results. Diameter and albedo 10μ radiometric data collected from Kitt Peak in 1975 gave a first diameter estimate of 209 km. According to the space-based surveys carried out by the Japanese Akari satellite, the Infrared Astronomical Satellite IRAS and the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, as well as observations by the Keck Observatory and photometric modeling, Camilla measures between 185 and 247 kilometers in diameter and its surface has an albedo between 0.160 and 0.294. Satellites Camilla is the 6th triple asteroid that has been discovered in the asteroid belt, after 87 Sylvia, 45 Eugenia, 216 Kleopatra, 93 Minerva and 130 Elektra (a quaternary). Outer satellite S/2001 (107) 1 #A0FFA0 yes A. Storrs, F. Vilas,R. Landis, E. Wells,C. Woods, B. Zellner,and M. Gaffey 1 March 2001 Pajuelo M. Carry B. Vachier F. Marsset M. Berthier J. Descamps P. Merline W.J. Tamblyn P.M. Grice J. Conrad A. Storrs A. Timerson B. Dunham D. Preston S. Vigan A. Yang B. Vernazza P. Fauvaud S. Bernasconi L. Romeuf D. Behrend R. Dumas C. Drummond J.D. Margot J.-L. Kervella P. Marchis F. Girard J.H. Physical, spectral, and dynamical properties of asteroid (107) Camilla and its satellites Icarus July 2018 309 134–161 10.1016/j.icarus.2018.03.003 1803.02722 2018Icar..309..134P 5642 days 1247.8 1.3 km 0.000 0.004 3.71234 0.00001 d 16.0 0.8 ° 12.7 3.5 km, assuming equal albedos and DCamilla = 254 km16 6 km~ 11 ± 2 km ~1.515 kgAssuming a similar density to the primary. 13.18 On 1 March 2001, a minor-planet moon of Camilla was found by A. Storrs, F. Vilas, R. Landis, E. Wells, C. Woods, B. Zellner, and M. Gaffey using the Hubble Space Telescope. It has the provisional designation S/2001 (107) 1 and has not received an official name. Later observations in September 2005 with the Very Large Telescope (VLT) allowed the determination of an orbit. In addition to the data in the infobox at right, the inclination was found to be 3 ± 1° with respect to an axis pointing towards (β, λ) = (+55°, 75°). Given the ~10° uncertainty in the actual rotational axis of Camilla, one can say that the orbit's inclination is less than 10°. The satellite is estimated to measure about 11 km in diameter. Assuming a similar density to the primary, this would give it an approximate mass of ~1.515 kg. It has a similar colour to the primary. Inner satellite S/2016 (107) 1 #A0FFA0 yes M. Marsset, B. Carry, B. Yang, F. Marchis, P. Vernazza, C. Dumas, J. Berthier, F. Vachier 29 May 2015 428 days 643.8 1.3 km 0.18 0.08 0.06 1.376 0.005 d 107 Camilla 27.7 7.3 ° 4.0 1.2 km, assuming equal albedos and DCamilla = 254 km In 2016, the discovery of a second satellite of Camilla was reported by astronomers at Cerro Paranal's Very Large Telescope in Chile. It has the provisional designation S/2016 (107) 1. Observations were taken between 29 May 2015 and 30 July 2016, using the VLT-SPHERE, the principal instrument attached to the 8-meter "Melipal" (UT3) unit of the VLT. On 3 out of 5 observation sessions, the new satellite could be detected. The body's orbit has a semi-major axis of 340 kilometers. Notes LCDB-Pietschnig-2011 Pietschnig (2011) web: Photometric observations from 28 March 2007. Rotation period 4.844 0.003 hours with a brightness amplitude of 0.47 magnitude. Quality code of 3. Summary figures at http://www.minorplanet.info/PHP/generateOneAsteroidInfo.php?AstInfo=107%7CCamilla Collaborative Asteroid Lightcurve Link (CALL) References 2018-02-07 last obs. JPL Small-Body Database Browser: 107 Camilla https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=2000107 Jet Propulsion Laboratory 7 July 2018 Schmadel Lutz D. Dictionary of Minor Planet Names Springer Berlin Heidelberg 25 2007 978-3-540-00238-3 10.1007/978-3-540-29925-7_108 (107) Camilla 107 Camilla Minor Planet Center https://www.minorplanetcenter.net/db_search/show_object?object_id=107 7 July 2018 IAUC 7599 6 M. Marsset B. Carry B. Yang F. Marchis P. Vernazza C. Dumas J. Berthier F. Vachier August 2016 S/2016 (107) 1 http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2016IAUC.9282....1M IAU Circ. 9282 1 2016IAUC.9282....1M 30 March 2017 Robert Johnston (107) Camilla, S/2001 (107) 1, and S/2016 (107) 1 johnstonsarchive.net 23 June 2015 http://www.johnstonsarchive.net/astro/astmoons/am-00107.html 30 March 2017 6 Joseph R. Masiero T. Grav A. K. Mainzer C. R. Nugent J. M. Bauer R. Stevenson S. 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Wolf February 2016 New and updated convex shape models of asteroids based on optical data from a large collaboration network Astronomy and Astrophysics 586 24 2016A&A...586A.108H 10.1051/0004-6361/201527441 free 1510.07422 119112278 D. Morrison C. R. Chapman March 1976 Radiometric diameters for an additional 22 asteroids http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=1976ApJ...204..934M Astrophysical Journal 204 934–939 1976ApJ...204..934M 10.1086/154242 31 March 2017 External links IAU Circulars – 2016: S/2016 (107) 1 (107) Camilla, S/2001 (107) 1, and S/2016 (107) 1, johnstonsarchive.net Hubble Finds New Asteroid Moon https://web.archive.org/web/20110514082634/http://www.spacedaily.com/news/asteroid-01c.html 14 May 2011 (SpaceDaily.com, 21–03–2001), includes discovery image. 107 Camilla and S/2001 (107) 1, orbit data website maintained by F. Marchis. Includes orbit diagrams. 107 106 Dione 107 108 Hecuba 000107 000107 Category:Discoveries by N. R. Pogson Category:Named minor planets 000107 000107 000107 18681117