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

From Wikipedia, the free encyclopedia

903 Nealley
Discovery
Discovered byJohann Palisa
Discovery siteVienna
Discovery date13 September 1918
Designations
(903) Nealley
1918 EM
Orbital characteristics[1]
Epoch 31 July 2016 (JD 2457600.5)
Uncertainty parameter 0
Observation arc97.59 yr (35646 days)
Aphelion3.3819 AU (505.93 Gm)
Perihelion3.0934 AU (462.77 Gm)
3.2377 AU (484.35 Gm)
Eccentricity0.044562
5.83 yr (2127.9 d)
229.469°
0° 10m 9.048s / day
Inclination11.781°
159.404°
235.383°
Earth MOID2.11158 AU (315.888 Gm)
Jupiter MOID1.84491 AU (275.995 Gm)
TJupiter3.150
Physical characteristics
Mean radius
31.715±1 km
21.60 h (0.900 d)
0.0528±0.004
10.0

903 Nealley is a minor planet orbiting the Sun. The semi-major axis of the orbit of 903 Nealley lies just inside the Hecuba gap, located at 3.27 AU.[2]

References

  1. ^ "903 Nealley (1918 EM)". JPL Small-Body Database. NASA/Jet Propulsion Laboratory. Retrieved 2 May 2016.
  2. ^ Scholl, Hans; Froeschlé, Claude (September 1975), "Asteroidal motion at the 5/2, 7/3 and 2/1 resonances", Astronomy and Astrophysics, 42 (3): 457–463, Bibcode:1975A&A....42..457S

External links


This page was last edited on 24 December 2023, at 15:22
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.