800 Kressmannia

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800 Kressmannia
800Kressmannia (Lightcurve Inversion).png
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[1] belonging to the Flora family in the Main Belt.[2] Its rotation period is 4.464 hours[2].

References[edit]

  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. 

External links[edit]