Web en Español

   

MAIN RESULTS

 


 

Our team has been working on the analysis of lunar impact flashes since 1997. During this period we have focused on different tasks:

   
Development of the observational technique (see e.g. Ortiz et al. 1999 and Ortiz et al. 2000).
   

Development of techniques for the analysis of these phenomena (see e.g. Bellot-Rubio et al. 2000a, Bellot-Rubio et al. 2000b, Madiedo et al. 2015).

   
Development of data acquisition and analysis software (see, e.g., Madiedo et al. 2015).
   

Systematic monitoring of the lunar surface from different astronomical observatories located in Spain.

   

Determination of impact plume temperatures since 2015 (Madiedo et al. 2016). Download here the poster presented at the Meteoroids 2016 Congress, held at ESTEC, the Netherlands.

   
Recording of the first lunar impact flash ever observed and confirmed during a lunar eclipse (Madiedo et al. 2019).

 

The September 11, 2013 impact event

Since our survey was started, we have recorded a large number of impact flashes produced by meteoroids belonging to the sporadic background and to different meteoroid streams (see some publications about this topic below). However, it is worth mentioning that two telescopes operated in the framework of MIDAS spotted on September 11, 2013 the brightest and longest (over 8 seconds in duration) lunar impact flash recorded so far (Madiedo et al. 2014). To date, no other survey has recorded a lunar impact blast larger than this.

 

Lunar impact flash recorded on September 11, 2013 in the framework of the MIDAS Project.

The crater produced by this event was located the by Lunar Reconnaissance Orbiter (LRO) probe in Mare Nubium. Despite the poor atmospheric transparency at the time of the observation, which made very difficult to identify features on the lunar surface to determine the selenographic coordinates of the impact position (see figure above), the location originally predicted by the MIDAS software for the new crater produced by this event differed from the position measured by LRO by only 2 km! This positional error is lower than the error determined by other surveys.

You can find below an outreach video produced on occasion of the publication of the analysis of this event in Monthly Notices of the Royal Astronomical Society:

 

 

Main publications in peer-reviewed journals

The following list contains some of the works published by us in the framework of the MIDAS Project:

*Ortiz, J.L., Aceituno, F.J., and Aceituno, J. (1999). A search for meteoritic flashes on the Moon. Astronomy and Astrophysics, 343, L57-L60.

*Ortiz, J.L., Aceituno, F.J., and Aceituno, J. (2000). Optical detection of meteoroidal impacts on the Moon. Nature, 405, 921-923.

*Bellot-Rubio, L.R., Ortiz, J.L., and Sada, P.V. (2000). Luminous Efficiency in Hypervelocity Impacts from the 1999 Lunar Leonids. The Astrophysical Journal, 542, L65-L68.
 

*Bellot-Rubio, L.R., Ortiz, J.L., and Sada, P.V. (2000). Observation and Interpretation of Meteoroid Impact Flashes on the Moon. Earth, Moon, and Planets, 82/83, 575-598.

 

*Ortiz, J.L., Quesada, J.A., Aceituno, J., Aceituno, F.J., and Bellot-Rubio, L.R. (2002). Observation and Interpretation of Leonid Impact Flashes on the Moon in 2001. The Astrophysical Journal, 576, 567-573.

 

*Ortiz, J.L., Aceituno, F.J., Quesada, J.A., Aceituno, J., Fernández, J., Santos-Sanz, P., Trigo-Rodríguez, J.M., Llorca, J., Martín-Torres, F.J., Montanes-Rodríguez, P., and Pallé, E. (2006). Detection of sporadic impact flashes on the
Moon: Implications for the luminous efficiency of hypervelocity impacts and derived terrestrial impact rates. Icarus, 184, 319-326.

 

*Madiedo, J.M., Trigo-Rodríguez, J.M., Ortiz, J.L., and Morales, N. (2010). Robotic Systems for Meteor Observing and Moon Impact Flashes Detection in Spain. Advances in Astronomy, Article ID 167494, 1-5.

 

*Madiedo, J.M., Ortiz, J.L., Morales, N., and Cabrera-Cano, J. (2014). A large lunar impact blast on 2013 September 11. Monthly Notices of the Royal Astronomical Society, 439, 2364-2369.
 

*Madiedo, J.M., Ortiz, J.L., Organero, F., Ana-Hernández, L., Fonseca, F., Morales, N., and Cabrera-Cano, J. (2015). Analysis of Moon impact flashes detected during the 2012 and 2013 Perseids. Astronomy and Astrophysics, 577, id.A118.


*Madiedo, J.M., Ortiz, J.L., Morales, N., and Cabrera-Cano, J. (2015). MIDAS: Software for the detection and analysis of lunar impact flashes. Planetary and Space Science, 111, 105-115.

*Ortiz, J.L., Madiedo, J.M., Morales, N., Santos-Sanz, P., and Aceituno, F.J., (2015). Lunar impact flashes from Geminids: analysis of luminous efficiencies and the flux of large meteoroids on Earth. Monthly Notices of the Royal Astronomical Society, 454, 344-352.

*Madiedo, J.M., Ortiz, J.L., and Morales, N. (2018). First determination of the temperature of a lunar impact flash and its evolution. Monthly Notices of the Royal Astronomical Society, 480, p.5010-5016.

*Madiedo, J.M., Ortiz, J.L., Morales, N. and Santos-Sanz, P. (2019). Multiwavelength observations of a bright impact flash during the 2019 January total lunar eclipse. Monthly Notices of the Royal Astronomical Society, 486, p.3380-3387.

 

 
   
  Web design and programming: J.M. Madiedo