37022 Robertovittori
Discovery[1][2] | |
---|---|
Discovered by | F. Manca and G. Ventre |
Discovery site | Sormano |
Discovery date | 22 October 2000 |
Designations | |
MPC designation | 37022 |
Named after | Roberto Vittori |
2000 UT1 | |
Orbital characteristics[1] | |
Epoch 13 January 2016 (JD 2457400.5) | |
Uncertainty parameter 0 | |
Observation arc | 6532 days (17.88 yr) |
Aphelion | 2.9677209 AU (443.96473 Gm) |
Perihelion | 2.6529491 AU (396.87554 Gm) |
2.8103350 AU (420.42013 Gm) | |
Eccentricity | 0.0560025 |
4.71 yr (1720.8 d) | |
66.335922° | |
0° 12m 33.129s / day | |
Inclination | 4.858204° |
180.40272° | |
251.67833° | |
Earth MOID | 1.6714 AU (250.04 Gm) |
Jupiter MOID | 2.19643 AU (328.581 Gm) |
Jupiter Tisserand parameter | 3.314 |
Proper orbital elements[2] | |
Proper semi-major axis | 2.80914 AU |
Proper eccentricity | 0.0521316 |
Proper mean motion | 76.443 deg / yr |
Proper orbital period |
4.70939 yr (1720.105 d) |
Precession of perihelion | 63.279 arcsec / yr |
Precession of the ascending node | -61.0255 arcsec / yr |
Physical characteristics | |
Dimensions | 8.341 km (5.183 mi)[3] |
0.25 (assumed) | |
Temperature | 155 K[4] |
14.3 | |
|
37022 Robertovittori (2000 UT1) is a main-belt asteroid discovered on October 22, 2000 by F. Manca and Graziano Ventre at Sormano. It is named after Roberto Vittori, an Italian astronaut who flew on multiple missions to the International Space Station.[1]
References
- 1 2 3 "37022 Robertovittori (2000 UT1)". JPL Small Body Database. JPL/NASA. October 2, 2003. Retrieved 12 April 2016.
- 1 2 "(37022) Robertovittori". Retrieved 14 October 2014.
- ↑ "Conversion of Absolute Magnitude to Diameter for Minor Planets". Stephen F. Austin State University. Dan Burton. Archived from the original on 23 July 2011. Retrieved 14 October 2014.
- ↑ "HEC: Exoplanets Calculator". Planetary Habitability Laboratory. University of Puerto Rico at Arecibo. Retrieved 14 October 2014.
External links
This article is issued from Wikipedia - version of the 9/29/2016. The text is available under the Creative Commons Attribution/Share Alike but additional terms may apply for the media files.