857 Glasenappia

In today's world, 857 Glasenappia is a topic that continues to generate interest and debate. Whether due to its impact on society, its relevance in popular culture or its importance in the scientific field, 857 Glasenappia continues to be the object of study and analysis around the world. From its origins to its influence today, 857 Glasenappia has left an indelible mark on history and its relevance continues today. In this article we will address different aspects related to 857 Glasenappia, exploring its different facets and its impact on the contemporary world.

857 Glasenappia
A three-dimensional model of 857 Glasenappia based on its light curve
Discovery
Discovered byS. Beljavskij
Discovery siteSimeis
Discovery date6 April 1916
Designations
(857) Glasenappia
Named after
Sergey Glazenap
1916 S33
Orbital characteristics[1]
Epoch 31 July 2016 (JD 2457600.5)
Uncertainty parameter 0
Observation arc95.56 yr (34905 days)
Aphelion2.3843 AU (356.69 Gm)
Perihelion1.9975 AU (298.82 Gm)
2.1909 AU (327.75 Gm)
Eccentricity0.088278
3.24 yr (1184.5 d)
232.96°
0° 18m 14.112s / day
Inclination5.2999°
82.932°
238.854°
Earth MOID0.989921 AU (148.0901 Gm)
Jupiter MOID2.81688 AU (421.399 Gm)
TJupiter3.662
Physical characteristics
7.515±0.35 km
8.23 h (0.343 d)
0.2318±0.024
11.32

857 Glasenappia is a minor planet orbiting the Sun. It was named after Russian astronomer Sergey Glazenap, who was often referred to as "S. de Glasenapp" in pre-Revolution publications.

References

  1. ^ "857 Glasenappia (1916 S33)". JPL Small-Body Database. NASA/Jet Propulsion Laboratory. Retrieved 4 May 2016.


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