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Published byDalibor Beránek Modified over 5 years ago
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Asteroidal Occultations during the rest of 2014 and during 2015
2014 July 13 32nd Annual IOTA Meeting University of Maryland Observatory College Park, MD David W. Dunham See
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SAO
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SAO
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SAO
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SAO
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2d after Solar Eclipse Conference
in Cloudcroft, NM
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SWRI Event SAO , sp. G5
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SWRI Event SAO 59412, sp. A5
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SWRI Event Asteroid maybe binary
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SAO , K5
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SWRI Binary asteroid
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SWRI lower priority
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SAO , K0
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SWRI event, binary asteroid
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SAO = ZC 736, sp. type F0
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ε [epsilon] Geminorum = Mebsuta = ZC 1030 = SAO 78682 = HIP 32246, sp
ε [epsilon] Geminorum = Mebsuta = ZC 1030 = SAO = HIP 32246, sp. G5. It will take at least 0.3s for the edge of Iphigenia to cover the angular diameter star. There will be 10-km-wide partial occultation zones centered on the edges of the 72-km-wide occultation path.
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IOTA meeting candidate,
but faint
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SWRI lower priority
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SWRI lower priority
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SAO , A2 IOTA meeting candidate
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SAO A0 IOTA meeting candidate; Last event shown
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