752 Sulamitis
| 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 | |
| 60.17±0.25 km[5] | |
| 27.367 h[6][7] | |
| 0.045±0.008[5] | |
| C (assumed)[6] | |
| 10.3[3] | |
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
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
- ^ a b c "752 Sulamitis (1913 RL)". Minor Planet Center. Retrieved 6 July 2018.
- ^ a b 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.
- ^ a b c "JPL Small-Body Database Browser: 752 Sulamitis (1913 RL)" (2018-05-25 last obs.). Jet Propulsion Laboratory. Retrieved 6 July 2018.
- ^ a b "Asteroid 752 Sulamitis". Small Bodies Data Ferret. Retrieved 6 July 2018.
- ^ a b 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.
- ^ a b "LCDB Data for (752) Sulamitis". Asteroid Lightcurve Database (LCDB). Retrieved 6 July 2018.
- ^ a b 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. pp. 297–321. arXiv:1502.01628. Bibcode:2015aste.book..297N. doi:10.2458/azu_uapress_9780816532131-ch016. ISBN 9780816532131.
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External links
- Discovery Circumstances: Numbered Minor Planets
- 752 Sulamitis at AstDyS-2, Asteroids—Dynamic Site
- 752 Sulamitis at the JPL Small-Body Database
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