Protoplanetary Disk tagged posts

Atmosphere of Midsize Planet revealed by Hubble, Spitzer

This artist’s illustration shows the theoretical internal structure of the exoplanet GJ 3470 b. It is unlike any planet found in the Solar System. Weighing in at 12.6 Earth masses the planet is more massive than Earth but less massive than Neptune. Unlike Neptune, which is 3 billion miles from the Sun, GJ 3470 b may have formed very close to its red dwarf star as a dry, rocky object. It then gravitationally pulled in hydrogen and helium gas from a circumstellar disk to build up a thick atmosphere. The disk dissipated many billions of years ago, and the planet stopped growing. The bottom illustration shows the disk as the system may have looked long ago...
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Carbonaceous Chondrites provide clues about the Delivery of Water to Earth

Carbonaceous chondrites provide clues about the delivery of water to Earth
Sample collecting of meteorites in Antarctica. Credit: Katherine Joy / ANSMET

Researchers have discovered that carbonaceous chondrites, a class of meteorites, incorporated hydrated minerals along with organic material from the protoplanetary disk before the formation of planets. Scientists from the study published in the journal Space Science Reviews note that these meteorites played “an important role in the primordial Earth’s water enrichment” because they facilitated the transportation of volatile elements that were accumulated on the external regions of the so-called protoplanetary disk from which planets were formed more than 4.500 years ago. Earth was formed in an environment close to the Sun, very much reduced due to the relative lack of oxygen.

Carbonaceous chondrites come fro...

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Diamond Dust Shimmering around Distant Stars

This is an artist impression of nanoscale diamonds surrounding a young star in the Milky Way. Recent GBT and ATCA observations have identified the telltale radio signal of diamond dust around 3 such stars, suggesting they are a source of the so-called anomalous microwave emission. Credit: S. Dagnello, NRAO/AUI/NSF

This is an artist impression of nanoscale diamonds surrounding a young star in the Milky Way. Recent GBT and ATCA observations have identified the telltale radio signal of diamond dust around 3 such stars, suggesting they are a source of the so-called anomalous microwave emission. Credit: S. Dagnello, NRAO/AUI/NSF

Nanoscale gemstones source of mysterious cosmic microwave light. Some of the tiniest diamonds in the universe – bits of crystalline carbon hundreds of thousands of times smaller than a grain of sand – have been detected swirling around 3 infant star systems in the Milky Way...

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Planet Formation: The Death of a Planet Nursery?

Planetary disk around the star known as TW Hydrae. Credit: S. Andrews (Harvard-Smithsonian CfA); B. Saxton (NRAO/AUI/NSF); ALMA (ESO/NAOJ/NRAO)

Planetary disk around the star known as TW Hydrae. Credit: S. Andrews (Harvard-Smithsonian CfA); B. Saxton (NRAO/AUI/NSF); ALMA (ESO/NAOJ/NRAO)

The dusty disk surrounding star TW Hydrae exhibits circular features that may signal the formation of protoplanets. An astrophysicist argues, however, that the innermost actually points to the impending dispersal of the disk. When the maps appeared at the end of March, experts were electrified. The images revealed an orange-red disk pitted with circular gaps: a detailed portrait of a protoplanetary disk, made up of gas and dust grains, associated with a young star – the kind of structure out of which planets could be expected to form...

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