Comets

The giant comet C/2014 UN271 (Bernardinelli-Bernstein)

The Las Cumbres Observatory has captured a new image of the giant comet C/2014 UN271 (Bernardinelli-Bernstein) that shows its activity despite its considerable distance given that it’s far beyond Saturn’s orbit. The information collected also by looking into archive images such as the ones that allowed to identify it in an image from 2014 is useful to better understand its characteristics. In particular, initial estimates suggested that its diameter was at least 100 kilometers, three times the largest known comet, but these are estimates based on the absence of a coma. C/2014 UN271 will remain far from the Sun, arriving close to Saturn’s orbit at the beginning of 2031, so it can only be admired with telescopes but it could still be very interesting because it probably comes from the Oort cloud.

Comet C/2016 R2 (PANSTARRS) and its spectrum (Image ESO/L. Calçada, SPECULOOS Team/E. Jehin, Manfroid et al.)

Two articles published in the journal “Nature” report different studies on the materials present in the atmospheres of comets, which appear to contain iron and nickel even in the ones far from the Sun. Jean Manfroid, Damien Hutsemekers, and Emmanuel Jehin used data collected by the UVES spectrograph of ESO’s VLT in Chile to analyze the atmospheres of various comets detecting the presence of both iron and nickel. Piotr Guzik and Michał Drahus used the X-shooter spectrograph, also of the VLT, to examine in particular the interstellar comet 2I/Borisov detecting the presence of nickel. They were surprising results because the sublimation of heavy metals was thought possible only near the Sun.

Comet P/2019 LD2 seen by Hubble (Image NASA, ESA, STScI, B. Bolin (IPAC/Caltech))

An article published in “The Astronomical Journal” reports a description of the characteristics of comet P/2019 LD2. A team of researchers used observations conducted with various space and ground-based telescopes to examine P/2019 LD2 while it’s passing near the planet Jupiter in a trajectory that brought it close to the Trojan asteroids to the point that it was initially mistaken for one of them.

The points of the various landings made by the lander Philae on the surface of comet 67P/Churyumov-Gerasimenko

An article published in the journal “Nature” reports a reconstruction of the trajectory of ESA’s Rosetta mission’s Philae lander in its touchdown on the surface of comet 67P/Churyumov-Gerasimenko. A team of researchers examined data collected by the Rosetta space probe and the Philae lander to find out where the latter made its second touchdown on the comet, which was followed by further bounces before finally landing. The study also showed that the affected materials contained an abundant amount of ice as soft as freshly laid snow, to the point of being described as softer than cappuccino froth.

Scheme of the CONSERT radar's work

An article published in the journal “Monthly Notices of the Royal Astronomical Society” reports a study indicating that the interior of the nucleus of comet 67P/Churyumov-Gerasimenko is porous and less dense than its surface. A team of researchers reviewed data collected by ESA’s Rosetta space probe and its Philae lander’s CONSERT instrument. The signals exchanged between them through the cometary nucleus propagated at different speeds, indicating a varying density of its interior. This suggests that solar radiation changed the surface, making it less porous.