Hovnatanian (crater)
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This is an old revision of this page, as edited by Drbogdan (talk | contribs) at 19:00, 2 November 2013 (added => {{Mercury (planet)}}). The present address (URL) is a permanent link to this revision, which may differ significantly from the current revision.
Hovnatanian is a crater on Mercury. Its “butterfly” pattern of ejecta rays were created by an impact at an even lower angle than that which formed neighboring Qi Baishi crater. From the "butterfly" pattern of rays, the Hovnatanian impactor was travelling either north-to-south or south-to-north prior to hitting Mercury's surface.[1]
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