The Observation of Lunar Impacts. Part II

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dc.creatorSigismondi, C.
dc.creatorImponente, G. P.
dc.date2001-05-14
dc.date.accessioned2026-07-07T01:58:34Z
dc.date.available2026-07-07T01:58:34Z
dc.descriptionThe frequency and the characteristics of lunar impacting meteorites are reconsidered under the general assumption of belonging to the sporadic meteoroids. We develop the model for evaluating the luminous energy detected in the visual band during the impact. The values obtained are consistent with the luminosity of an Earth's meteor as seen at the Moon's distance, although we recover significantly smaller magnitudes for the lunar impacts with respect to other authors.
dc.description3 pages
dc.identifierhttps://arxiv.org/abs/astro-ph/0105226
dc.identifierhttp://arxiv.org/abs/astro-ph/0105226
dc.identifierWGN, Journal of the International Meteor Organization, vol. 28, no. 6, p. 230-232, 12/2000
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/2767
dc.subjectAstrophysics
dc.titleThe Observation of Lunar Impacts. Part II
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