665 Sabine

665 Sabine
	A three-dimensional model of 665 Sabine based on its light curve
Discovery
Discovered by	W. Lorenz
Discovery site	Heidelberg
Discovery date	22 July 1908
Designations
MPC designation	(665) Sabine
Pronunciation	German: [zaːˈbiːnə][1]
Alternative designations	1908 DK
Adjectives	Sabinian /səˈbɪniən/[2]
Orbital characteristics[3]
	Epoch 31 July 2016 (JD 2457600.5)
	Uncertainty parameter 0
Observation arc	110.08 yr (40208 d)
Aphelion	3.6830 AU (550.97 Gm)
Perihelion	2.6053 AU (389.75 Gm)
Semi-major axis	3.1442 AU (470.37 Gm)
Eccentricity	0.17139
Orbital period (sidereal)	5.58 yr (2036.4 d)
Mean anomaly	149.933°
Mean motion	0° 10m 36.444s / day
Inclination	14.740°
Longitude of ascending node	298.436°
Argument of perihelion	318.920°
Physical characteristics
Mean radius	25.545±1.2 km[3]; 26.355 ± 0.36 km[4]
Mass	(6.98 ± 3.98) × 1017 kg[4]
Synodic rotation period	4.294 h (0.1789 d)
Geometric albedo	0.3895±0.039
Absolute magnitude (H)	9.29,[5] 8.7[3]

665 Sabine is a minor planet orbiting the Sun that was discovered by German astronomer Wilhelm Lorenz on July 22, 1908.[6]

Photometric observations of this asteroid at the Oakley Observatory in Terre Haute, Indiana during 2006 gave a light curve with a period of 4.294 ± 0.001 hours and a brightness variation of 0.50 ± 0.04 in magnitude.[7]

References

(German Names)
"Sabinian". Oxford English Dictionary (Online ed.). Oxford University Press. (Subscription or participating institution membership required.)
Yeomans, Donald K., "665 Sabine", JPL Small-Body Database Browser, NASA Jet Propulsion Laboratory, retrieved 7 May 2016.
Carry, B. (December 2012), "Density of asteroids", Planetary and Space Science, vol. 73, pp. 98–118, arXiv:1203.4336, Bibcode:2012P&SS...73...98C, doi:10.1016/j.pss.2012.03.009. See Table 1.
Warner, Brian D. (December 2007), "Initial Results of a Dedicated H-G Project", The Minor Planet Bulletin, vol. 34, pp. 113–119, Bibcode:2007MPBu...34..113W.
"Numbered Minor Planets 1–5000", Discovery Circumstances, IAU Minor Planet center, retrieved 7 April 2013.
Ditteon, Richard; Hawkins, Scot (September 2007), "Asteroid Lightcurve Analysis at the Oakley Observatory - October-November 2006", The Minor Planet Bulletin, vol. 34, no. 3, pp. 59–64, Bibcode:2007MPBu...34...59D.

External links

665 Sabine at AstDyS-2, Asteroids—Dynamic Site
- Ephemeris · Observation prediction · Orbital info · Proper elements · Observational info
665 Sabine at the JPL Small-Body Database

This article is issued from Wikipedia. The text is licensed under Creative Commons - Attribution - Sharealike. Additional terms may apply for the media files.

[1] (German Names)

[2] "Sabinian". Oxford English Dictionary (Online ed.). Oxford University Press. (Subscription or participating institution membership required.)

[JPL-3] Yeomans, Donald K., "665 Sabine", JPL Small-Body Database Browser, NASA Jet Propulsion Laboratory, retrieved 7 May 2016.

[Carry2012-4] Carry, B. (December 2012), "Density of asteroids", Planetary and Space Science, vol. 73, pp. 98–118, arXiv:1203.4336, Bibcode:2012P&SS...73...98C, doi:10.1016/j.pss.2012.03.009. See Table 1.

[Warner2007-5] Warner, Brian D. (December 2007), "Initial Results of a Dedicated H-G Project", The Minor Planet Bulletin, vol. 34, pp. 113–119, Bibcode:2007MPBu...34..113W.

[IAU_MPC-6] "Numbered Minor Planets 1–5000", Discovery Circumstances, IAU Minor Planet center, retrieved 7 April 2013.

[Warner2008-7] Ditteon, Richard; Hawkins, Scot (September 2007), "Asteroid Lightcurve Analysis at the Oakley Observatory - October-November 2006", The Minor Planet Bulletin, vol. 34, no. 3, pp. 59–64, Bibcode:2007MPBu...34...59D.