800 Kressmannia
A three-dimensional model of 800 Kressmannia based on its light curve. | |
Discovery | |
---|---|
Discovered by | Max Wolf |
Discovery site | Heidelberg |
Discovery date | 20 March 1915 |
Designations | |
1915 WP; A905 CF; A912 GC | |
Orbital characteristics[1] | |
Epoch 31 July 2016 (JD 2457600.5) | |
Uncertainty parameter 0 | |
Observation arc | 104.01 yr (37991 d) |
Aphelion | 2.6341 AU (394.06 Gm) |
Perihelion | 1.7512 AU (261.98 Gm) |
2.1926 AU (328.01 Gm) | |
Eccentricity | 0.20134 |
3.25 yr (1185.9 d) | |
316.007° | |
0° 18m 12.852s / day | |
Inclination | 4.2623° |
325.184° | |
347.603° | |
Earth MOID | 0.736953 AU (110.2466 Gm) |
Jupiter MOID | 2.63325 AU (393.929 Gm) |
Jupiter Tisserand parameter | 3.641 |
Physical characteristics | |
4.464 h (0.1860 d) | |
11.61 | |
|
800 Kressmannia is an S-type asteroid belonging to the Flora family in the Main Belt.[2] Its rotation period is 4.464 hours.
References
- ↑ "800 Kressmannia (1915 WP)". JPL Small-Body Database. NASA/Jet Propulsion Laboratory. Retrieved 4 May 2016.
- ↑ Kryszczynska, A.; et al. (October 2012). "Do Slivan states exist in the Flora family?. I. Photometric survey of the Flora region". Astronomy & Astrophysics. 546: 51. Bibcode:2012A&A...546A..72K. doi:10.1051/0004-6361/201219199. A72.
External links
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