February 2016

Artistic representation of the WFIRST Space Telescope (Image NASA/GSFC/Conceptual Image Lab)

NASA announced the approval of a new astrophysics mission based on a space telescope called WFIRST (Wide-Field Infrared Survey Telescope). It’s a next-generation Instrument for a long-term project since it will be probably launched around the middle of next decade. It will have a mirror as large as Hubble’s but a field of view a hundred times wider to investigate even better on the secrets of the universe.

The Astro-H space telescope blasting off atop an H-IIA rocket (Image courtesy JAXA)

A little while ago the Japanese Astro-H space telescope was launched from the Tanegashima Space Center on a H-IIA rocket. After about fifteen minutes it regularly separated from the rocket’s last stage. It will reach the low-Earth orbit, where it will be positioned at an altitude of about 575 kilometers (about 357 miles).

The Sentinel-3A blasting off atop a Rockot launch vehicle (Photo ESA)

A few hours ago the Sentinel-3A satellite, part of the GMES / Copernicus program, was launched from the Russian Plesetsk Cosmodrome on a Rockot launch vehicle. After about an hour and a half it separated from the rocket’s last stage, called Breeze KM, it started communicating with the control center and to deploy its solar panels. Its final orbit is Sun-synchronous, which means it will pass over a certain area of ​​the Earth at the same local time, with an altitude of about 815 kilometers (about 506 miles).

An image of the HD 142527 binary star system from observations made with the ALMA radio telescope (Image Andrea Isella/Rice University; B. Saxton (NRAO/AUI/NSF); ALMA (NRAO/ESO/NAOJ)

At the meeting of the AAAS (American Association for the Advancement of Science) just concluded in Washington, D.C. the latest results were presented about the observations of the HD 142527 star system carried out with the ALMA radio telescope. It’s been an object of study by astronomers for some time and is particularly interesting because it’s very young. This means that around the central star there’s a ring of gas and dust that is probably forming one or more planets but there’s also a second star. This type of study will help to understand the formation of planets in binary systems.

Artist's impression of the Philae lander (Image ESA–J. Huart)

The hopes to be able to contact the lander Philae on the comet 67P/Churyumov-Gerasimenko’s surface have now faded and ESA is also pessimistic. DLS, the German space agency, runs the LCC (Lander Control Center) and in recent months tried to re-establish contact after Philae communicated for a while on several occasions but issued a statement declaring that it’s time to say goodbye to the lander.