Astronomy:2014 SC324

From HandWiki
Revision as of 16:56, 19 July 2022 by imported>Scavis2 (link)
(diff) ← Older revision | Latest revision (diff) | Newer revision → (diff)
2014 SC324
Discovery[1]
Discovered byMt. Lemmon Survey (G96)
Discovery date30 September 2014
Designations
2014 SC324
Minor planet category
Orbital characteristics[2]
Epoch 13 January 2016 (JD 2457400.5)
Uncertainty parameter 1
Observation arc29 days w/Radar
|{{{apsis}}}|helion}}2.93880 astronomical unit|AU (439.638 Gm) (Q)
|{{{apsis}}}|helion}}0.91503 AU (136.887 Gm) (q)
1.92691 AU (288.262 Gm) (a)
Eccentricity0.52513 (e)
Orbital period2.67 yr (976.99 d)
Mean anomaly152.737° (M)
Mean motion0° 22m 6.521s / day (n)
Inclination1.65403° (i)
Longitude of ascending node210.19563° (Ω)
221.35334° (ω)
Earth MOID0.000606726 AU (90,764.9 km)
Physical characteristics
Dimensions37–85 m (generic)[3]
Rotation period0.36156 h (21.694 min)
Apparent magnitude24-29 (2014–2015)
Absolute magnitude (H)24.3[2]


2014 SC324 is a sub-kilometer asteroid and fast rotator, classified as a near-Earth object of the Apollo group, approximately 50 meters in diameter.[2] It was first observed on 30 September 2014, by the Mount Lemmon Survey at an apparent magnitude of 21 using a 1.5-meter (59 in) reflecting telescope.[1] With an absolute magnitude of 24.3,[2] the asteroid is about 37–85 meters in diameter.[3]

Description

The preliminary orbit with a short observation arc of 2 days showed that the asteroid had a very small chance of passing 0.000125 astronomical unit|AU (18,700 km; 11,600 mi) from the Moon or 0.0012 AU (180,000 km; 110,000 mi) from Earth on about 23 October 2014.[4] But with an observation arc of 10 days, the nominal (best fit) orbit showed that on 24 October 2014 the asteroid would pass 0.0038 AU (570,000 km; 350,000 mi) (1.5 LD) from Earth and even further from the Moon.[5] The asteroid peaked at apparent magnitude 13.5,[6] placing it in the range of amateurs with roughly 0.25-meter (10 in) telescopes.

It was removed from the Sentry Risk Table on 10 October 2014 using JPL solution #5 with a 10-day observation arc.[7]

It was observed by Goldstone radar on 24–25 October 2014.[8]

References

External links