To install click the Add extension button. That's it.

The source code for the WIKI 2 extension is being checked by specialists of the Mozilla Foundation, Google, and Apple. You could also do it yourself at any point in time.

4,5
Kelly Slayton
Congratulations on this excellent venture… what a great idea!
Alexander Grigorievskiy
I use WIKI 2 every day and almost forgot how the original Wikipedia looks like.
What we do. Every page goes through several hundred of perfecting techniques; in live mode. Quite the same Wikipedia. Just better.
.
Leo
Newton
Brights
Milds

857 Glasenappia

From Wikipedia, the free encyclopedia

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
Mean radius
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.

External links


This page was last edited on 14 January 2024, at 20:42
Basis of this page is in Wikipedia. Text is available under the CC BY-SA 3.0 Unported License. Non-text media are available under their specified licenses. Wikipedia® is a registered trademark of the Wikimedia Foundation, Inc. WIKI 2 is an independent company and has no affiliation with Wikimedia Foundation.