2007 CA19

2007 CA19
Discovery
Discovered by Catalina Sky Survey
Discovery date February 11, 2007
Designations
none
Apollo asteroid,
Earth-crosser asteroid
Mars-crosser asteroid
Orbital characteristics[1]
Epoch 13 January 2016 (JD 2457400.5)
Uncertainty parameter 0
Observation arc 3258 days (8.92 yr)
Aphelion 5.11769 AU (765.596 Gm)
Perihelion 0.502914 AU (75.2349 Gm)
2.81030 AU (420.415 Gm)
Eccentricity 0.821046
4.71 yr (1720.8 d)
306.543°
 12m 33.142s /day
Inclination 9.58919°
170.154°
102.390°
Earth MOID 0.0193363 AU (2.89267 Gm)
Jupiter MOID 0.817257 AU (122.2599 Gm)
Physical characteristics
Dimensions 0.864 km
Mass 8.9×1011 kg
Mean density
2.6 g/cm³
17.6

    2007 CA19 (also written 2007 CA19) is a near-Earth asteroid. It led the impact hazard list, with a Torino Scale impact risk value of 1, for one week, ending on February 19, 2007. Before and after 2007 CA19, 99942 Apophis was the object with the highest Palermo Scale rating. With an observation arc of 4.8 days, 2007 CA19 had a Palermo Scale of −0.88.[2]

    2007 CA19 was discovered on February 11, 2007 by the Catalina Sky Survey at the University of University of Arizona. The object is estimated at 966 metres in diameter with a mass of a 1.2x1012 kg. Until February 15, it had an impact probability of 1/625000 for the day March 14, 2012.[2] Additional observations through February 19 decreased the impact probability to ~1 in 300 million, making it of negligible concern. It was removed from the Sentry Risk Table on February 22, 2007.[3]

    2007 CA19 passed about 0.007 AU (1,000,000 km; 650,000 mi) from Venus on July 6, 1946.[1]

    See also

    References

    1. 1 2 "JPL Close-Approach Data: (2007 CA19)". Retrieved 30 March 2016. 2008-02-14 last obs (arc=5.85 yr)
    2. 1 2 "Earth Impact Risk Summary: 2007 CA19". Wayback Machine: NASA/JPL Near-Earth Object Program Office. Archived from the original on February 16, 2007. (1.6e-06 = 1 in 625,000 chance)
    3. "Date/Time Removed". NASA/JPL Near-Earth Object Program Office. Retrieved 2013-07-27.

    External links

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