planetesimals tagged posts

To Stick or to Bounce: Size determines the Stickiness of Cosmic Dust Aggregates

Micrometer-scale dust particles from protoplanetary disks, or sites around stars with particles and hydrogen and/or other gasses, aggregate to form planetesimals, or kilometer-scale building blocks of planets. Planetesimals, in turn, merge due to mutual gravity. ©JAMSTEC

Microparticle dust aggregates, which are thought to play a role in the formation of new planets, are less likely to stick together after a collision when the aggregates are larger.

Current evidence suggests that microparticles of cosmic dust collide and stick together to form larger dust aggregates that may eventually combine and develop into planets...

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Where did Earth’s Water come from? Not Melted Meteorites, according to scientists

The dashed white line in this illustration shows the boundary between the inner solar system and outer solar system, with the asteroid belt positioned roughly in between Mars and Jupiter. A bubble near the top of the image shows water molecules attached to a rocky fragment, demonstrating the kind of object that could have carried water to Earth. Credit: Jack Cook/Woods Hole Oceanographic Institution. Click image to download hi-res version.

Water makes up 71% of Earth’s surface, but no one knows how or when such massive quantities of water arrived on Earth.

A new study published in the journal Nature brings scientists one step closer to answering that question...

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Unknown Class of Water-Rich Asteroids Identified

Unknown of water-rich asteroids identified
Implantation of planetesimals into the asteroid belt during the planets’ growth and dynamical evolution. Credit: Nature Astronomy (2023). DOI: 10.1038/s41550-023-01898-x

New astronomical measurements in the infrared range have led to the identification of a heretofore unknown class of asteroids. An international research team including geoscientists from Heidelberg University has succeeded in characterizing these small planets using infrared spectroscopy.

They are located in the asteroid belt between Mars and Jupiter and are—similar to the dwarf planet Ceres—rich in water. According to computer models, complex dynamic processes shifted these asteroids from the outer regions of our solar system into today’s asteroid belt shortly after their creation.

With an equatorial diame...

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Cosmic History can explain the Properties of Mercury, Venus, Earth and Mars

This is the sharpest image ever taken by ALMA — sharper than is routinely achieved in visible light with the NASA/ESA Hubble Space Telescope. It shows the protoplanetary disc surrounding the young star HL Tauri. These new ALMA observations reveal substructures within the disc that have never been seen before and even show the possible positions of planets forming in the dark patches within the system. Credit: ALMA (ESO/NAOJ/NRAO)

Astronomers have managed to link the properties of the inner planets of our solar system with our cosmic history: with the emergence of ring structures in the swirling disk of gas and dust in which these planets were formed...

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