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=Forsberg, Herrick, and Bussey (1998): The Effects of Impact Angle on the Shape of Lunar Craters=
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==Description==
 Paper differentiates [[Oblique%20Impact%20Craters|oblique]] versus high-angle (vertical) impacts by comparing down-range and cross-range profiles. The crater profiles were extracted from the Apollo [[LTO|LTO]] charts.<br /> <br /> 
==Additional Information==
* Craters identified as high-angle based on symmetric profiles are: [[Timocharis|Timocharis]], [[Fischer|Fischer]], '''[[Macrobius|Macrobius]] A''', [[Peek|Peek]] and [[Sulpicius%20Gallus|Sulpicius Gallus]]
* Craters identified as low-angle (unsymmetric) are [[Necho|Necho]], [[Proclus|Proclus]], [[Pytheas|Pytheas]], '''[[Messier|Messier]] A''', and [[Messier|Messier]]
* [[Messier|Messier]] is identified as likely a 1° impact with '''[[Messier|Messier]] A''' as a ricochet product.
* '''[[Torricelli|Torricelli]] A''' (not illustrated) and [[Pytheas|Pytheas]] are identified as likely 15° impacts. The remaining unsymmetric craters are believed to be from impacts in the range 15° to 45°.
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==LPOD Articles==
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==Bibliography==
 Forsberg, N. K.; Herrick, R. R.; Bussey, B. 1998. [http://adsabs.harvard.edu/abs/1998LPI....29.1691F The Effects of Impact Angle on the Shape of Lunar Craters]. 29th Annual Lunar and Planetary Science Conference, March 16-20, 1998, Houston, TX, abstract no. 1691.<br /> <br /> <br />
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