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arxiv: 1905.04487 · v1 · pith:P3AHXZ27new · submitted 2019-05-11 · 🌌 astro-ph.EP

Multiwavelength observations of a bright impact flash during the January 2019 total lunar eclipse

classification 🌌 astro-ph.EP
keywords flashimpactlunareclipseduringobservationscircfirst
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We discuss here a lunar impact flash recorded during the total lunar eclipse that occurred on 2019 January 21, at 4h 41m 38.09 +- 0.01 s UT. This is the first time ever that an impact flash is unambiguously recorded during a lunar eclipse and discussed in the scientific literature, and the first time that lunar impact flash observations in more than two wavelengths are reported. The impact event was observed by different instruments in the framework of the MIDAS survey. It was also spotted by casual observers that were taking images of the eclipse. The flash lasted 0.28 seconds and its peak luminosity in visible band was equivalent to the brightness of a mag. 4.2 star. The projectile hit the Moon at the coordinates 29.2 +- 0.3 $^{\circ}$S, 67.5 +- 0.4 $^{\circ}$W. In this work we have investigated the most likely source of the projectile, and the diameter of the new crater generated by the collision has been calculated. In addition, the temperature of the lunar impact flash is derived from the multiwavelength observations. These indicate that the blackbody temperature of this flash was of about 5700 K.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. Mare versus highland lunar impact flash light curve dichotomy

    astro-ph.EP 2026-05 unverdicted novelty 5.0

    Lunar impact flashes on highlands exhibit shallower, longer-lasting decay than on mare terrain, driven by fine ejecta in dual-size cooling models and indicating lithology-dependent early cratering.

  2. Mare versus highland lunar impact flash light curve dichotomy

    astro-ph.EP 2026-05 unverdicted novelty 5.0

    Lunar impact flashes on highlands exhibit longer and shallower decay than on maria, with the dual-size ejecta model attributing the difference mainly to fine droplets and indicating lithology dependence in early cratering.