A little while ago a GSLV Mk-III rocket blasted off from the Indian Satish Dhawan Space Centre with the Chandrayaan 2 mission’s orbiter, the Vikram lander and the Pragyaan rover. After just over 16 minutes, the vehicles separated from the rocket’s last stage to begin the series of maneuvers that will slowly stretch their orbit to bring them into the area of influence of the Moon, where the lander and rover’s landing is scheduled as soon as September 6.
A few hours ago the Soyuz MS-13 spacecraft was launched from the Baikonur Cosmodrome in Kazakhstan and after a little more than six hours reached the International Space Station with three astronauts on board: Drew Morgan, Alexander Skvortsov and Luca Parmitano.
On July 20, 1969, NASA’s Apollo 11 mission’s lunar module Eagle, started on July 16, accomplished the first Moon landing of a manned spacecraft. Mission commander Neil Armstrong and lunar module pilot Edwin “Buzz” Aldrin participated in the landing and spent just over two hours on the surface of the Moon to collect some samples that were brought back to Earth. Once they departed the Moon, the two astronauts rejoined Michael Collins, who remained in orbit in the command module Columbia and returned to Earth on July 24th.
An article being published in “The Astrophysical Journal” reports a new attempt to calculate the speed of the universe expansion, this time using red giant stars as a reference. A team of researchers coordinated by Carnegie Institution for Science and University of Chicago and led by astronomer Wendy Freedman used observations made with the Hubble space telescope to perform that calculation. The result has a probability peak at 69.8 km/s per megaparsec, between the values calculated using the two methods that provided discrepant values.
An article published in the journal “Nature” offers a possible explanation of the remarkable difference in the presence of some chemical elements on the Earth and on the Moon still accepting the theory of their common origin following an impact with the primordial Earth. A team of researchers carried out a series of simulations of the impacts that could have happened on the Moon during the first phase of its history, concluding that the retention of the elements classified as highly siderophilous began 4.35 billion years ago, at the time when most of the magma that covered the lunar surface solidified.