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 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 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°
Physical characteristics
Mean diameter
15 km
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 .

    Related Research Articles

    References

    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.