800 Kressmannia is an S-type asteroid[1] belonging to the Flora family in the Main Belt.[2] Its rotation period is 4.464 hours[2].

800 Kressmannia
A three-dimensional model of 800 Kressmannia based on its light curve
Discovery
Discovered byMax Wolf
Discovery siteHeidelberg Observatory
Discovery date20 March 1915
Designations
(800) Kressmannia
Pronunciation/krɛsˈmæniə/
1915 WP; A905 CF;
A912 GC
Orbital characteristics[1]
Epoch 31 July 2016 (JD 2457600.5)
Uncertainty parameter 0
Observation arc104.01 yr (37991 d)
Aphelion2.6341 AU (394.06 Gm)
Perihelion1.7512 AU (261.98 Gm)
2.1926 AU (328.01 Gm)
Eccentricity0.20134
3.25 yr (1185.9 d)
316.007°
0° 18m 12.852s / day
Inclination4.2623°
325.184°
347.603°
Physical characteristics
15 km
4.464 h (0.1860 d)
11.61

References

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  1. ^ "800 Kressmannia (1915 WP)". JPL Small-Body Database. NASA/Jet Propulsion Laboratory. Retrieved 4 May 2016.
  2. ^ 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.
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