Protoplanetary Disk tagged posts

The only way astronomers have been able to detect rogue planets is through microlensing events caused by the slight gravitational effect of an object on background light. This occurs when the light from a distant star suddenly appears magnified to an observer (telescopes on Earth), as if a lens were placed in front of it. The magnification of light lets astronomers know that something has passed in front of the distant star.

Theoretically, microlensing can allow for the calculation of the mass of the object passing in front of the star by analyzing how much the light was bent and thus magnified...

Using the Atacama Large Millimeter/submillimeter Array (ALMA), a team of astronomers led by Abubakar Fadul from the Max Planck Institute for Astronomy (MPIA) has discovered complex organic molecules—including the first tentative detection of ethylene glycol and glycolonitrile—in the protoplanetary disk of the outbursting protostar V883 Orionis.

These compounds are considered precursors to the building blocks of life. Comparing different cosmic environments reveals that the abundance and complexity of such molecules increase from star-forming regions to fully evolved planetary systems. This suggests that the seeds of life are assembled in space and are widespread.

The findings are published in the Astrophysical Journal Letters.

Astronomers have discovered complex organic m...

Identifying the formation period of planetary systems, such as our solar system, could be the beginning of the journey to discover the origin of life. The key to this is the unique substructures found in protoplanetary disks—the sites of planet formation.

A protoplanetary disk is composed of low-temperat...