752 Sulamitis
752 Sulamitis /suːləˈmaɪtɪs/ is an asteroid from the inner regions of the asteroid belt, approximately 60 kilometers (37 miles) in diameter. It is the parent body of the Sulamitis family (408),[4] a small family of 300 known carbonaceous asteroids.[8]:23
Discovery [1] | |
---|---|
Discovered by | G. Neujmin |
Discovery site | Simeiz Obs. |
Discovery date | 30 April 1913 |
Designations | |
(752) Sulamitis | |
Pronunciation | /suːləˈmaɪtɪs/ |
Named after | Shulamite (Hebrew Bible)[2] |
1913 RL · 1936 FH1 | |
main-belt [1][3] · (inner) Sulamitis [4] | |
Orbital characteristics [3] | |
Epoch 23 March 2018 (JD 2458200.5) | |
Uncertainty parameter 0 | |
Observation arc | 101.01 yr (36,894 d) |
Aphelion | 2.6457 AU |
Perihelion | 2.2795 AU |
2.4626 AU | |
Eccentricity | 0.0743 |
3.86 yr (1,412 d) | |
149.88° | |
0° 15m 18s / day | |
Inclination | 5.9617° |
85.120° | |
23.880° | |
Physical characteristics | |
Mean diameter | 60.17±0.25 km[5] |
27.367 h[6][7] | |
0.045±0.008[5] | |
C (assumed)[6] | |
10.3[3] | |
Sulamitis was discovered on 30 April 1913 by Georgian–Russian astronomers Grigory Neujmin at the Simeiz Observatory on the Crimean peninsula, and given the provisional designation 1913 RL.[1] It was named after the Shulamite, a beautiful woman mentioned in the book Solomon's Song of Songs of the Old Testament. The figure in possibly the Queen of Sheba in the Hebrew Bible.[2]
Photometric observations of this asteroid collected during 2004–2005 show a rotation period of 27.367 ± 0.005 hours with a brightness variation of 0.20 ± 0.03 magnitude.[7]
References
- "752 Sulamitis (1913 RL)". Minor Planet Center. Retrieved 6 July 2018.
- Schmadel, Lutz D. (2007). "(752) Sulamitis". Dictionary of Minor Planet Names – (752) Sulamitis. Springer Berlin Heidelberg. pp. 71–72. doi:10.1007/978-3-540-29925-7_753. ISBN 978-3-540-00238-3.
- "JPL Small-Body Database Browser: 752 Sulamitis (1913 RL)" (2018-05-25 last obs.). Jet Propulsion Laboratory. Retrieved 6 July 2018.
- "Asteroid 752 Sulamitis". Small Bodies Data Ferret. Retrieved 6 July 2018.
- Masiero, Joseph R.; Grav, T.; Mainzer, A. K.; Nugent, C. R.; Bauer, J. M.; Stevenson, R.; et al. (August 2014). "Main-belt Asteroids with WISE/NEOWISE: Near-infrared Albedos". The Astrophysical Journal. 791 (2): 11. arXiv:1406.6645. Bibcode:2014ApJ...791..121M. doi:10.1088/0004-637X/791/2/121.
- "LCDB Data for (752) Sulamitis". Asteroid Lightcurve Database (LCDB). Retrieved 6 July 2018.
- Pray, Donald P. (September 2005), "Lightcurve analysis of asteroids 106, 752, 847, 1057, 1630, 1670, 1927 1936, 2426, 2612, 2647, 4087, 5635, 5692, and 6235", The Minor Planet Bulletin, 32 (3): 48–51, Bibcode:2005MPBu...32...48P.
- 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.
External links
- Discovery Circumstances: Numbered Minor Planets
- 752 Sulamitis at AstDyS-2, Asteroids—Dynamic Site
- 752 Sulamitis at the JPL Small-Body Database