A few hours ago, the Tianwen-2 mission was successfully launched. A Long March 3B rocket blasted off from the Xichang Satellite Launch Center, and after about 18 minutes, the space probe separated from the rocket’s last stage to begin its journey towards the asteroid 469219 Kamoʻoalewa. The goal is to collect samples from its surface to bring back to Earth and then resume its journey in space towards the comet 311P/PanSTARRS.
It was the afternoon in the USA when SpaceX conducted a new flight test of its Super Heavy rocket and Starship prototypes, launched from its base in Boca Chica, Texas. This is the 9th test involving the entire system of Elon Musk’s company, which is supposed to revolutionize space travel with an unprecedented transport capacity and being totally reusable. They are advanced prototypes with the Super Heavy identified as Booster 14, on its second flight in the first reuse of a Super Heavy, and the Starship Block 2 identified as Starship 35 or Ship35 or simply S35.
A few hours ago, SpaceX’s Dragon spacecraft ended its CRS-32 (Cargo Resupply Service 32) mission for NASA splashing down smoothly off the coast of California. The Dragon left the International Space Station about 36 hours earlier. For SpaceX, this was the 12th mission of the 2nd contract with NASA to transport supplies to the Station with the new version of the Dragon cargo spacecraft. The Dragon spacecraft had reached the International Space Station on April 22.
An article published in “The Astrophysical Journal Letters” reports the results of a study of the Small Magellanic Cloud that shows how this dwarf galaxy is undergoing distortions in its shape due to various gravitational influences. Satoya Nakano and Kengo Tachihara of Nagoya University, Japan, used data collected by ESA’s Gaia space probe together with information on Cepheid stars collected by the OGLE (Optical Gravitational Lensing Experiment) project. This allowed them to determine the distances of 4,236 Cepheids and the anomalies in their motions. The conclusion is that the Small Magellanic Cloud is undergoing a gravitational influence from the Large Magellanic Cloud and another as yet unknown source.
An article to be published in the journal “Astronomy & Astrophysics” reports a study of the supernova SN 1987A that offers evidence that the explosion was decidedly asymmetric and dominated by two bipolar jets. A team of researchers led by astrophysicist Salvatore Orlando of the Italian National Institute of Astrophysics in Palermo has developed a model that takes into account the interaction between matter and magnetic field to study the evolution of SN 1987A. The results successfully reproduce the morphology of the iron-rich ejected materials, which was observed in particular by the James Webb Space Telescope. This shows that those structures are the result of an asymmetric explosion.
