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

DOI: 
10.1051/0004-6361/201525656
Publication date: 
01/05/2015
Main author: 
Madiedo J.M.
IAA authors: 
Ortiz J.L.;Morales N.
Authors: 
Madiedo J.M., Ortiz J.L., Organero F., Ana-Hernández L., Fonseca F., Morales N., Cabrera-Caño J.
Journal: 
Astronomy and Astrophysics
Publication type: 
Article
Volume: 
577
Pages: 
Number: 
A118
Abstract: 
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 × 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. © ESO, 2015.
Database: 
WOK
SCOPUS
ADS
SCOPUS
URL: 
https://ui.adsabs.harvard.edu/#abs/2015A&A...577A.118M/abstract
ADS Bibcode: 
2015A&A...577A.118M
Keywords: 
Meteorites, meteors, meteoroids; Moon