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Research reveals secret shared by comets and sand crabs

The study reveals that sand crabs build narrow burrows to prevent collapse, with the upper limit of stable burrow widths being around 5 cm. The researchers also found that cometary pits have a similar lower size limit, suggesting that both are governed by the same principle: the mechanics of cohesive granular matter.

SourceNagoya University·JournalScientific Reports·DateOct 25, 2018

ESO's VLT sees `Oumuamua getting a boost

Researchers found that `Oumuamua is venting material from its surface due to solar heating, causing a tiny boost in speed. This outgassing behavior is typical for comets and contradicts the previous classification of `O'uamua as an interstellar asteroid.

SourceESO·JournalNature·DateJun 27, 2018

Is the interstellar asteroid really a comet?

A team of astronomers led by Marco Micheli and Karen Meech found that Oumuamua was not slowing down due to gravitational forces alone, pointing to non-gravitational perturbations similar to those experienced by comets. Despite initial classification as an asteroid, the object's trajectory and behavior are more consistent with a comet.

Experiments at Berkeley Lab help trace interstellar dust back to solar system's formation

Researchers at Berkeley Lab used infrared light and electron microscopy to study interplanetary particles, finding they contain pre-solar dust leftover from the solar system's formation. The dust, consisting of carbon, ices, and disordered silicate, was mostly destroyed by planet formation processes.

SourceDOE/Lawrence Berkeley National Laboratory·JournalProceedings of the National Academy of Sciences·DateJun 11, 2018

Comet Chury formed by a catastrophic collision

A team of researchers proposes a new scenario for the formation of Comet Chury, suggesting it formed through a gentle encounter between two comets, preserving its primordial composition. This process allows for the survival of small bodies like Chury, which would otherwise be destroyed by collisions in the regions where they orbit.

SourceCNRS·JournalNature Astronomy·DateMar 6, 2018

Zwicky Transient Facility sees 'first light'

The Zwicky Transient Facility's (ZTF) new survey camera captures hundreds of thousands of stars and galaxies in a single shot, taking its first image of the sky, dubbed 'first light.' ZTF aims to discover objects and events varying in brightness over time, including explosive supernovae, hungry black holes, and asteroids/comets.

Comet mission reveals 'missing link' in our understanding of planet formation

Researchers from Germany's Technische Universität Braunschweig uncovered a crucial link between the formation of cometary 'dust pebbles' and planet accretion. The study, based on Rosetta mission data, reveals that these pebbles are concentrated by solar instability, leading to collapse and the birth of comets.

SourceRoyal Astronomical Society·JournalMonthly Notices of the Royal Astronomical Society·DateOct 25, 2017

Indicator of extraterrestrial life?

Researchers have discovered Freon-40, an organohalogen, around two celestial objects: an infant star and a comet. The finding suggests that these molecules may form readily in stellar nurseries, providing insights into the chemical evolution of planetary systems.

SourceUniversity of Cologne·JournalNature Astronomy·DateOct 4, 2017

ALMA and Rosetta detect Freon-40 in space

Researchers detected Freon-40, a stable organohalogen molecule, around infant star system IRAS 16293-2422 and comet 67P/C-G using ALMA and Rosetta. This finding suggests that organohalogens may be an important element in the origin of life, rather than indicators of existing life.

SourceESO·JournalNature Astronomy·DateOct 2, 2017

Does the organic material of comets predate our solar system?

A recent study published in Monthly Notices of the Royal Astronomical Society reveals that comet nuclei contain 40% organic matter by mass, which was produced in interstellar space before the formation of our solar system. This finding has significant implications for the origin of life on Earth and potentially other planets.

SourceCNRS·JournalMonthly Notices of the Royal Astronomical Society·DateSep 6, 2017