Analysis of Moon impact flashes detected during the 2012 and 2013 Perseids

被引:26
作者
Madiedo, Jose M. [1 ,2 ]
Ortiz, Jose L. [3 ]
Organero, Faustino [4 ]
Ana-Hernandez, Leonor [4 ]
Fonseca, Fernando [4 ]
Morales, Nicolas [3 ]
Cabrera-Cano, Jesus [1 ]
机构
[1] Univ Seville, Fac Fis, Dept Fis Atom Mol & Nucl, E-41012 Seville, Spain
[2] Univ Huelva, Fac Ciencias Expt, Huelva 21071, Spain
[3] CSIC, Inst Astrofis Andalucia, E-18080 Granada, Spain
[4] Observ Astron La Hita, La Puebla De Almoradiel 45071, Toledo, Spain
关键词
meteorites; meteors; meteoroids; Moon; METEOROID STREAM; HYPERVELOCITY IMPACTS; LUMINOUS EFFICIENCY; ORIONID; ORBITS; SYSTEM;
D O I
10.1051/0004-6361/201525656
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present the results of our Moon impact flash detection campaigns performed around the maximum activity period of the Perseid meteor shower in 2012 and 2013. Just one flash produced by a Perseid meteoroid was detected in 2012 because of very unfavorable geometric conditions, but 12 flashes were confirmed in 2013. The visual magnitude of the flashes ranged between 6.6 and 9.3. A luminous efficiency of 1.8 x 10(-3) has been estimated for meteoroids from this stream. According to this value, impactor masses would range between 1.9 and 190 g. In addition, we propose a criterion for establishing, from a statistical point of view, the likely origin of impact flashes recorded on the lunar surface.
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页数:9
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