903 Nealley
Appearance
(Redirected from Nealley)
Discovery | |
---|---|
Discovered by | Johann Palisa |
Discovery site | Vienna |
Discovery date | 13 September 1918 |
Designations | |
(903) Nealley | |
1918 EM | |
Orbital characteristics[1] | |
Epoch 31 July 2016 (JD 2457600.5) | |
Uncertainty parameter 0 | |
Observation arc | 97.59 yr (35646 days) |
Aphelion | 3.3819 AU (505.93 Gm) |
Perihelion | 3.0934 AU (462.77 Gm) |
3.2377 AU (484.35 Gm) | |
Eccentricity | 0.044562 |
5.83 yr (2127.9 d) | |
229.469° | |
0° 10m 9.048s / day | |
Inclination | 11.781° |
159.404° | |
235.383° | |
Earth MOID | 2.11158 AU (315.888 Gm) |
Jupiter MOID | 1.84491 AU (275.995 Gm) |
TJupiter | 3.150 |
Physical characteristics | |
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
[edit]- ^ "903 Nealley (1918 EM)". JPL Small-Body Database. NASA/Jet Propulsion Laboratory. Retrieved 2 May 2016.
- ^ 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
[edit]- Lightcurve plot of 903 Nealley, Palmer Divide Observatory, B. D. Warner (2011)
- Asteroid Lightcurve Database (LCDB), query form (info Archived 16 December 2017 at the Wayback Machine)
- Dictionary of Minor Planet Names, Google books
- Asteroids and comets rotation curves, CdR – Observatoire de Genève, Raoul Behrend
- Discovery Circumstances: Numbered Minor Planets (1)-(5000) – Minor Planet Center
- 903 Nealley at AstDyS-2, Asteroids—Dynamic Site
- 903 Nealley at the JPL Small-Body Database