Massimo Luciani

The capsule containting asteroid Bennu's samples (Image NASA TV)

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A little while ago, the samples taken from the asteroid Bennu brought back to Earth by NASA’s OSIRIS-REx space probe were collected by the American space agency’s crew in the area of their landing, at the Utah Test and Training Range. They will be transported to the Johnson Space Center, the first stage of a series of operations needed to process them while avoiding their contamination. In this study, NASA is collaborating with the Japanese space agency JAXA, which will receive some of the samples to compare them with those collected by its own Hayabusa 2 space probe on the asteroid Ryugu and returned to Earth in December 2020.

Arp 107 (Image ESA/Hubble & NASA, J. Dalcanton)

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An image captured by the Hubble Space Telescope shows Arp 107, a pair of interacting galaxies heading towards a collision. The two galaxies, the spiral galaxy UGC 5984 (or PGC 32620) and the elliptical galaxy MCG +05-26-025 (or PGC 32628), will finish this process in a merger. UGC 5984 is a Seyfert galaxy, a class characterized by an active galactic nucleus that doesn’t block the view of the rest of the galaxy and spectral lines that show a strong ionization. The pair represents an interesting case of the early phase of a galaxy merger.

The HIP 81208 system seen by SPHERE

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An article published in the journal “Astronomy & Astrophysics” reports the discovery of an object that could be a gas giant planet or a brown dwarf in the HIP 81208 system. A team of researchers analyzed data from the archive of the observations conducted with the SPHERE instrument mounted on the VLT in Chile discovering an object that was cataloged as HIP 81208 Cb orbiting the smaller of the two stars in this binary system. A brown dwarf was discovered around the more massive star together with the smaller and more distant star in an analysis also published some time ago in an article in “Astronomy & Astrophysics”. The new discovery makes HIP 81208 a so-called hierarchical quadruple system, the first of its kind discovered using a direct imaging system.

The Soyuz MS-24 spacecraft blasting off atop a Soyuz-2.1a rocket (Image NASA TV)

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A few hours ago, the Soyuz MS-24 spacecraft was launched from the Baikonur Cosmodrome in Kazakhstan and after a little more than three hours reached the International Space Station with three new crew members on board. It docked with the Station’s Rassvet module. As is becoming increasingly common for crewed trips as well, the ultra-fast track was used which halves the journey duration.

Oleg Kononenko and Nikolai Chub will spend about a year on the International Space Station while Loral O’Hara will spend about six months there and return to Earth with different traveling companions. Expedition 69 is almost over, as in less than two weeks, the crew members who’ve been on the Station for a year will return to Earth marking the start of Expedition 70.

A diagram illustrating the combined power of the James Webb and Hubble space telescopes in studying Cepheids present in the galaxy NGC 5584 with the NIRCam (Near-Infrared Camera) and WFC3 (Wide Field Camera 3) instruments, respectively

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An article accepted for publication in “The Astrophysical Journal” reports the results of calculating the universe’s expansion rate based on the observation of Cepheids with the James Webb Space Telescope. In particular, a team of researchers led by Adam Riess used the NIRCam instrument to observe over 330 cepheids in the galaxies NGC 4258 and NGC 5584. The results are more precise than those obtained in the past with the Hubble Space Telescope but confirm the accuracy of the previous calculation of the universe’s expansion rate. This leaves open the question of the difference in results obtained with different methods.