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(196256) 2003 EH1
Near-Earth asteroid
Near-Earth asteroid
| Field | Value | |
|---|---|---|
| minorplanet | yes | |
| background | #FFC2E0 | |
| name | ||
| discovery_ref | ||
| discoverer | LONEOS | discovered = 6 March 2003 |
| mpc_name | ||
| mp_category | NEOAmor | |
| extinct comet | ||
| orbit_ref | ||
| epoch | 13 January 2016 (JD 2457400.5) | |
| eccentricity | 0.618907 (e) | |
| semimajor | 3.12275 AU (a) | |
| perihelion | 1.190060 AU (q) | |
| period | 5.52 yr (2015.6 d) | |
| aphelion | 5.055446 AU (Q) | |
| inclination | 70.865968° (i) | |
| asc_node | 282.972499° (Ω) | |
| abs_magnitude | 16.2 | |
| dimensions | 2.6 – | |
| albedo | 0.04–0.09 (assumed) | |
| arg_peri | 171.3709° (ω) | |
| mean_anomaly | 119.8736° (M) | |
| mean_motion | / day (n) | |
| observation_arc | 4035 days (11.05 yr) | |
| uncertainty | 0 | |
| moid | 0.21143 AU | |
| jupiter_moid | 0.231939 AU | |
| tisserand | 2.065 | |
| sidereal_day |
extinct comet
**** is an asteroid, classified as a near-Earth object of the Amor group. It was discovered on 6 March 2003, by astronomers of the LONEOS program at Anderson Mesa Station near Flagstaff, Arizona, in the United States. Peter Jenniskens (2003–2004) proposed that it is the parent body of the Quadrantid meteor shower. is likely an extinct comet and may even be related to the comet C/1490 Y1. came to perihelion on 12 March 2014. thumb|320px|left|The orbit of
References
References
- (2015). "Physical Observations of (196256) 2003 EH1, Presumed Parent of the Quadrantid Meteoroid Stream". The Astronomical Journal.
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