752 Sulamitis

752 Sulamitis
Discovery
Discovered by	G. Neujmin
Discovery site	Simeiz Obs.
Discovery date	30 April 1913
Designations
MPC designation	(752) Sulamitis
Pronunciation	/suːləˈmaɪtɪs/
Named after	Shulamite; (Hebrew Bible)
Alternative designations	1913 RL · 1936 FH1
Minor planet category	main-belt · (inner); Sulamitis
Orbital characteristics
	Epoch 23 March 2018 (JD 2458200.5)
	Uncertainty parameter 0
Observation arc	101.01 yr (36,894 d)
\|{{{apsis}}}\|helion}}	2.6457 astronomical unit\|AU (395.79 Gm)
\|{{{apsis}}}\|helion}}	2.2795 AU (341.01 Gm)
Semi-major axis	2.4626 AU (368.40 Gm)
Eccentricity	0.0743
Orbital period	3.87 yr (1,412 d)
Mean anomaly	149.88°
Mean motion	0° 15m 18s / day
Inclination	5.9617°
Longitude of ascending node	85.120°
\|{{{apsis}}}\|helion}}	23.880°
Physical characteristics
Mean diameter	60.17±0.25 km
Rotation period	27.367 h
Geometric albedo	0.045±0.008
Spectral type	C (assumed)
Absolute magnitude (H)	10.3

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 This asteroid is orbiting 2.46 astronomical unit|AU from the Sun with a period of 3.87 years and an eccentricity of 0.0743. The orbital plane is inclined at an angle of 5.96° to the plane of the ecliptic.^[3]

Sulamitis was discovered on 30 April 1913 by Georgian–Russian astronomer 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 is 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 h with a brightness variation of 0.20±0.03 magnitude.^[7] A hydration feature in the spectrum of 752 Sulamitis indicates the surface has undergone aqueous alteration. The same feature appears in most of its family members, suggesting the original body held water in some form.^[9]

References

↑ ^1.0 ^1.1 ^1.2 "752 Sulamitis (1913 RL)". Minor Planet Center. https://www.minorplanetcenter.net/db_search/show_object?object_id=752.
↑ ^2.0 ^2.1 Schmadel, Lutz D. (2007). "(752) Sulamitis". Dictionary of Minor Planet Names. Springer Berlin Heidelberg. pp. 71–72. doi:10.1007/978-3-540-29925-7_753. ISBN 978-3-540-00238-3.
↑ ^3.0 ^3.1 ^3.2 ^3.3 "JPL Small-Body Database Browser: 752 Sulamitis (1913 RL)". Jet Propulsion Laboratory. https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=2000752.
↑ ^4.0 ^4.1 "Asteroid 752 Sulamitis". Small Bodies Data Ferret. https://sbntools.psi.edu/ferret/SimpleSearch/results.action?targetName=752+Sulamitis.
↑ ^5.0 ^5.1 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. doi:10.1088/0004-637X/791/2/121. Bibcode: 2014ApJ...791..121M.
↑ ^6.0 ^6.1 "LCDB Data for (752) Sulamitis". Asteroid Lightcurve Database (LCDB). http://www.minorplanet.info/PHP/generateOneAsteroidInfo.php?AstInfo=752|Sulamitis.
↑ ^7.0 ^7.1 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. doi:10.2458/azu_uapress_9780816532131-ch016. ISBN 9780816532131. Bibcode: 2015aste.book..297N.
↑ Morate, David et al. (February 2018), "Visible spectroscopy of the Sulamitis and Clarissa primitive families: a possible link to Erigone and Polana", Astronomy & Astrophysics 610: 14, doi:10.1051/0004-6361/201731407, A25, Bibcode: 2018A&A...610A..25M.

External links

Discovery Circumstances: Numbered Minor Planets
752 Sulamitis at AstDyS-2, Asteroids—Dynamic Site
- Ephemeris · Observation prediction · Orbital info · Proper elements · Observational info
752 Sulamitis at the JPL Small-Body Database
- Close approach · Discovery · Ephemeris · Orbit diagram · Orbital elements · Physical parameters

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Original source: https://en.wikipedia.org/wiki/752 Sulamitis. Read more

[MPC-object-1] 1.0 ^1.1 ^1.2 "752 Sulamitis (1913 RL)". Minor Planet Center. https://www.minorplanetcenter.net/db_search/show_object?object_id=752.

[springer-2] 2.0 ^2.1 Schmadel, Lutz D. (2007). "(752) Sulamitis". Dictionary of Minor Planet Names. Springer Berlin Heidelberg. pp. 71–72. doi:10.1007/978-3-540-29925-7_753. ISBN 978-3-540-00238-3.

[jpldata-3] 3.0 ^3.1 ^3.2 ^3.3 "JPL Small-Body Database Browser: 752 Sulamitis (1913 RL)". Jet Propulsion Laboratory. https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=2000752.

[Ferret-4] 4.0 ^4.1 "Asteroid 752 Sulamitis". Small Bodies Data Ferret. https://sbntools.psi.edu/ferret/SimpleSearch/results.action?targetName=752+Sulamitis.

[Masiero-2014-5] 5.0 ^5.1 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. doi:10.1088/0004-637X/791/2/121. Bibcode: 2014ApJ...791..121M.

[lcdb-6] 6.0 ^6.1 "LCDB Data for (752) Sulamitis". Asteroid Lightcurve Database (LCDB). http://www.minorplanet.info/PHP/generateOneAsteroidInfo.php?AstInfo=752|Sulamitis.

[BMPS32_3_48-7] 7.0 ^7.1 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.

[Nesvorny-2014-8] Nesvorný, D.; Broz, M.; Carruba, V. (December 2014). "Identification and Dynamical Properties of Asteroid Families". Asteroids IV. pp. 297–321. doi:10.2458/azu_uapress_9780816532131-ch016. ISBN 9780816532131. Bibcode: 2015aste.book..297N.

[Morate_et_al_2018-9] Morate, David et al. (February 2018), "Visible spectroscopy of the Sulamitis and Clarissa primitive families: a possible link to Erigone and Polana", Astronomy & Astrophysics 610: 14, doi:10.1051/0004-6361/201731407, A25, Bibcode: 2018A&A...610A..25M.