105 Artemis

Main-belt asteroid October 2019 yes #D6D6D6 105 Artemis Орбита астероида 105.png Orbital diagram James Craig Watson 16 September 1868 (105) Artemis A868 SA ' ɑːr t ə m ə sArtemis Artemis Artemidean / Artemidian ɑːr t ə ' m ɪ d i ə nSophocles (1902 trans.)Dowden (1989) Death and the maiden: girls' initiation rites in Greek mythology Artemisian ɑːr t ə ' m ɪ z i ə nFischer-Hansen & Poulsen (2009) From Artemis to Diana Main belt 31 July 2016 (JD 2457600.5) 2.37319 AU Gm on 1.95119 AU Gm on 2.7952 AU Gm on on 0.17782 3.66 yr (1335.4 d) 21.444° 188.264° 57.077° 256.90° 19.18 km/s 119.08 2.8 km (1.54 ± 0.54) × 1018 kg 1.73 ± 0.67 g/cm3 0.0333 m/s² 0.0630 km/s 37.15506 h d on on37.15 h C (Tholen)Ch (Bus) 8.57 0.0465 0.002 ~180 K 0.26959 ms / day 100.79 yr (36812 d) 0 1.00955 AU Gm on 2.31243 AU Gm on 3.430 105 Artemis is a main-belt asteroid that was discovered by J. C. Watson on September 16, 1868, at Ann Arbor, Michigan. It was named after Artemis, the goddess of the hunt, Moon, and crossways in Greek mythology. It is a C-type asteroid, meaning that it is very dark and composed of carbonaceous material. Although it shares a similar orbit to the Phocaea family of S-type asteroids, its classification means 105 Artemis is not a member. The spectra of the asteroid displays evidence of aqueous alteration. In 1988, this object was detected with radar from the Arecibo Observatory at a distance of 1.07 AU. The measured radar cross-section was 1,800 km2. Photometric measurement of this asteroid made in 2010 at Organ Mesa Observatory in Las Cruces, New Mexico, produced an irregular light curve with a period of 37.150 ± 0.001 hours. During each rotation, the brightness varies by 0.16 ± 0.01 in magnitude. Based upon radar data, the estimated near surface solid density of the asteroid is 3.00.9 0.8 g cm−3. Refined observations by the Arecibo Observatory, reported in 2006, showed a complex surface with varying albedo. Analysis of the spectra of 105 Artemis shows the presence of hydrated minerals at some rotation angles, but not at others. An occultation of the star HD 197999 was observed in 1982, which gave an estimated chord length of 110 km. Between 1981 and 2021, 105 Artemis has been observed to occult 23 stars. References E. F. Tedesco P. V. Noah M. Noah S. D. Price October 2004 IRAS Minor Planet Survey V6.0 https://sbnarchive.psi.edu/pds3/iras/IRAS_A_FPA_3_RDR_IMPS_V6_0/data/diamalb.tab NASA Planetary Data System 12 IRAS-A-FPA-3-RDR-IMPS-V6.0 2004PDSS...12.....T 22 October 2019 Donald K. Yeomans 105 Artemis JPL Small-Body Database Browser NASA Jet Propulsion Laboratory https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=105 12 May 2016 . Spectroscopic comparison of aqueous altered asteroids with CM2 carbonaceous chondrite meteorites 1 . Fornasier S. Lazzarin M. Barbieri C. Barucci M. A. Astronomy and Astrophysics Supplement 135 65–73 February 1999 10.1051/aas:1999161 1999A&AS..135...65F free Schmade Lutz Dictionary of Minor Planet Names 1 Springer 5th 2003 25 3540002383 https://books.google.com/books?id=KWrB1jPCa8AC&pg=PA25 . Ostro S. J. Jurgens R. F. Rosema K. D. Winkler R. Yeomans D. K. Campbell D. B. Chandler J. F. Shapiro I. I. Hine A. A. Velez R. 1 Asteroid radar astrometry Astronomical Journal 102 1490–1502 October 1991 1991AJ....102.1490O 10.1086/115975 . Pilcher Frederick New Lightcurves of 40 Harmonia and 105 Artemis The Minor Planet Bulletin 37 4 167 October 2010 2010MPBu...37..167P . Byrne P. B. Coulson I. M. Doyle J. G. Taylor G. E. 1 Observations of the occultation of HD 197999 by the minor planet 105 Artemis Monthly Notices of the Royal Astronomical Society 200 65P–68P September 1982 1982MNRAS.200P..65B . 10.1093/mnras/200.1.65p free Carruba Valerio Rosa D. A. 1 An Analysis of the Region of the Phocaea Dynamical Family American Astronomical Society, DPS meeting #41, #27.04 September 2009 2009DPS....41.2704C http://www.feg.unesp.br/~vcarruba/phocaea.pdf 2013-03-18 . Magri C. Consolmagno G. J. Ostro S. J. Benner L. A. M. Beeney B. R. 1 Radar constraints on asteroid regolith compositions using 433 Eros as ground truth Meteoritics & Planetary Science 36 12 1697–1709 December 2001 10.1111/j.1945-5100.2001.tb01857.x 2001M&PS...36.1697M . Hanson Heather M. Howell E. S. Magri C. Nolan M. C. 1 Correlating Arecibo Radar and IRTF Near-Infrared Spectral Observations of 105 Artemis Bulletin of the American Astronomical Society 38 933 December 2006 2006AAS...209.2504H . B. Carry Density of asteroids Planetary and Space Science 73 98–118 December 2012 10.1016/j.pss.2012.03.009 2012P&SS...73...98C . 1203.4336 See Table 1. Francesca E. DeMeo Richard P. Binzel Stephen M. Slivan Schelte J. Bus 1 An extension of the Bus asteroid taxonomy into the near-infrared Icarus 202 1 160–180 2011 10.1016/j.icarus.2009.02.005 2009Icar..202..160D http://www.tara.tcd.ie/bitstream/2262/43276/1/PEER_stage2_10.1016%252Fj.icarus.2009.02.005.pdf 2013-03-22 . dead https://web.archive.org/web/20140317200310/https://www.tara.tcd.ie/bitstream/2262/43276/1/PEER_stage2_10.1016/j.icarus.2009.02.005.pdf 2014-03-17 See appendix A. External links 105 104 Klymene 105 106 Dione 000105 Category:Discoveries by James Craig Watson Category:Named minor planets 000105 000105 000105 18680916