Formation of a sub-lunar disk
Supplementary video of the paper "A multiple-impact origin for the Moon," authored by Raluca Rufu, Oded Aharonson & Hagai B. Perets, published in Nature Geoscience (2017) doi:10.1038/ngeo2866. Received 14 September 2016 Accepted 30 November 2016 Published online 09 January 2017
http://dx.doi.org/10.1038/ngeo2866
Example of formation of a sub-lunar disk. The 0.025 impactor
has a velocity of 2 time the escape velocity, at an impact angle of 30 degrees, and a fast initial planetary rotation of 0.5 ω max. The color bars represent the entropy of the impactor and target. The movie captures the equatorial plane cross-section and the two parts overlap for display reasons. To emphasis the merging of the cores, the impactor core is shown over the target. The Roche limit is represented by the dashed line.
Смотрите видео Formation of a sub-lunar disk онлайн без регистрации, длительностью часов минут секунд в хорошем качестве. Это видео добавил пользователь Francis Villatoro 11 Январь 2017, не забудьте поделиться им ссылкой с друзьями и знакомыми, на нашем сайте его посмотрели 1,94 раз и оно понравилось 1 людям.