(523775) 2014 YB35: Difference between revisions
Content deleted Content added
m added link |
No edit summary |
||
Line 1: | Line 1: | ||
{{orphan|date=March 2015}} |
|||
{{DISPLAYTITLE:2014 YB<sub>35</sub>}} |
{{DISPLAYTITLE:2014 YB<sub>35</sub>}} |
||
{{Infobox planet |
{{Infobox planet |
Revision as of 23:52, 14 March 2015
Discovery[1] | |
---|---|
Discovered by | Catalina Sky Survey |
Discovery date | 2014 Dec 27 |
Designations | |
Designation | 2014 YB35 |
Apollo NEO[2] | |
Orbital characteristics[2] | |
Observation arc | 76 days |
Aphelion | 2.780 AU (Q) |
Perihelion | 0.9694 AU (q) |
1.875 AU (a) | |
Eccentricity | 0.4829 |
2.57 yr | |
316.2° (M) | |
Inclination | 12.651° |
3.797° | |
188.7° | |
Physical characteristics | |
Dimensions | ~500 meters[1] |
18.9[2] | |
2014 YB35 (also written 2014 YB35) is a near-Earth asteroid on the order of 500 meters in diameter. It was discovered on 2014 Dec 27 by the Catalina Sky Survey.[1] It will pass earth on 2015 Mar 27 at a distance of 4,473,807 +/- 155 km (0.03 AU, 11.7 lunar orbits); relative speed, 10.2 km/sec.[2]
Goldstone is scheduled to observe this object on Mar 20 and they expect to obtain coarse radar images as well as continuous wave (CW) spectra, which will indicate composition.
2014 YB35 will pass Earth again at a slightly closer distance in 2033, and again in 2128.
List_of_asteroid_close_approaches_to_Earth_in_2015
References
- ^ a b c "Goldstone Radar Observations Planning: 2002 FG7 and 2014 YB35". Jet Propulsion Laboratory. 2015-03-04. Retrieved 2015-03-13. (K14Y35B)
- ^ a b c d "JPL Small-Body Database Browser: 2014 YB35". Jet Propulsion Laboratory. 2015-03-13. Retrieved 2015-03-13. (K14Y35B)