2014 SC324

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]

2014 SC324
Discovery[1]
Discovered byMt. Lemmon Survey (G96)
Discovery date30 September 2014
Designations
2014 SC324
Orbital characteristics[2]
Epoch 13 January 2016 (JD 2457400.5)
Uncertainty parameter 1
Observation arc29 days w/Radar
Aphelion2.93880 AU (439.638 Gm) (Q)
Perihelion0.91503 AU (136.887 Gm) (q)
1.92691 AU (288.262 Gm) (a)
Eccentricity0.52513 (e)
2.67 yr (976.99 d)
152.737° (M)
 22m 6.521s / day (n)
Inclination1.65403° (i)
210.19563° (Ω)
221.35334° (ω)
Earth MOID0.000606726 AU (90,764.9 km)
Physical characteristics
Dimensions37–85 m (generic)[3]
0.36156 h (21.694 min)
24-29 (2014–2015)
24.3[2]

    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 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]

    gollark: This avoids the problems of proof of stake/work, but does mean you get some authority controlling it, which is... well, the situation now?
    gollark: We have... several thousand of them.
    gollark: What would probably be neat is cryptocurrency-type tech, except with new money added by having it be signed by some authority instead.
    gollark: Perhaps. Though one assumes they could probably do better.
    gollark: Though presumably they could *technically* just OCR the details off the card?

    References

    1. "MPEC 2014-T10 : 2014 SC324". IAU Minor Planet Center. 2 October 2014. Retrieved 2 October 2014. (K14SW4C)
    2. "JPL Small-Body Database Browser: (2014 SC324)" (last observation: 2014-10-29; arc: 29 days). Jet Propulsion Laboratory. Retrieved 4 April 2016.
    3. "Absolute Magnitude (H)". NASA/JPL. Retrieved 2 October 2014.
    4. Webcite capture of JPL solution #1 for asteroid 2014 SC324 on 2014-Oct-02
      ArchiveToday capture of JPL solution #1 for asteroid 2014 SC324 on 2014-Oct-02. url: N4eGm
    5. "JPL Close-Approach Data: (2014 SC324)" (last observation: 2014-10-29; arc: 29 days). Retrieved 10 October 2014.
    6. "2014SC324 Ephemerides for 23 October 2014 and 24 October 2014". NEODyS (Near Earth Objects  Dynamic Site). Retrieved 24 October 2014.
    7. "Date/Time Removed". NASA/JPL Near-Earth Object Program Office. Retrieved 10 October 2014.
    8. Dr. Lance A. M. Benner. "Goldstone Radar Observations Planning: 2340 Hathor, 2014 SM143, 2014 RQ17, 2014 TV, and 2014 SC324". NASA/JPL Asteroid Radar Research. Retrieved 30 October 2014.


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