Tomorrow, May 29, 2012 at about 07:07 UT, the asteroid designated 2012 KT42 will pass only ~14,000 km (8,700 miles) or about ~0.05 lunar distance (or 0.0001379 AU) above the Earth’s surface. The asteroid was discovered by Mt. Lemmon Survey with a 1.5-m reflector + CCD on May 28, 2012 at magnitude ~18.1.
According to its absolute magnitude (H=28.8) this asteroid has an estimated size of roughly 3-10 meters, so it is a small object. We have been able to follow-up this object soon after his discovery while it was still on the neocp, from the Siding Spring-Faulkes Telescope South on 2012, May 28.4, through a 2.0-m f/10.0 Ritchey-Chretien + CCD.
At the moment of our images from FTS, “2012 KT42” was moving at about ~3.63 “/min and its magnitude was ~17.5. At the moment of its close approach around 07UT of tomorrow, 2012 KT42 will be bright as magnitude ~12.0 and moving at ~11021″/min.
Below you can see an image (stack of 5×5-second exposures) showing the asteroid. Click on the thumbnail to see a bigger version:
Here you can see an animation showing the motion of 2012 KT42. Each frame is a 5-second exposure through the FTS 2.0-m telescope.
While there is no cause for concern, this is one of the closest approaches recorded. The table below shows the top 20 closest approaches by NEOs (Near-Earth Objects) sorted by nominal distance. The table has been computed on the NASA/Neo-JPL website. 2012 KT42 is the sixth closer approach to date. (2011 CQ1 is the closest non-impacting object in the asteroid catalog to date. The event that took 2008 TC3 into the earth’s atmosphere is not included). Click on the thumbnail to see a bigger version:
On mpml mailing list, Andrew Lowe pointed out that on May 29 at about 10:10 UT, 2012 KT42 the minimum geocentric elongation from the center of the sun will be 0.1 degrees, so given the parallax there will be a transit across the sun, centered in southern Asia. If the diameter is about 5m, then the object could be only about 0.006″ across against the solar disk. Aldo Vitagliano provided this map of the transit (computed by his software Solex). Click on the thumbnail to see a bigger version:
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