All astronomers concur that planets are created in protoplanetary disks, which are the bands of gas and dust that encircle newly-formed young stars. Even though the universe has hundreds of these disks, it has been challenging to observe genuine planetary birth and development in these settings.

Currently, astronomers at the Center for Astrophysics, Harvard and Smithsonian, have created a novel method to find these elusive newborn planets, along with “smoking gun” proof of a small Neptune- or Saturn-like planet hiding in a disk. The Astrophysical Journal Letters on Thursday published a description of the findings.

According to Feng Long, a postdoctoral scholar at the Center for Astrophysics and project leader, “directly finding young planets is highly tough and has so far only been effective in one or two situations.”

As they are encased in substantial amounts of gas and dust, planets are always too dim for us to see them.

Instead, they must look for signs that a planet is forming beneath the dust. Long notes that in recent years, “many structures have appeared on disks that we think are caused by the existence of a planet but it could be caused by something else too.” “We need new methods to examine and provide evidence that a planet exists.”

Long chose to revisit the LkCa 15 protoplanetary disk for her research. The disc is situated in the Taurus constellation, 518 light years away. Previous research employing ALMA Observatory images showed proof of planet formation in the disk. Long dug over fresh, high-resolution ALMA data on LkCa 15, mostly from 2019, and found two faint characteristics that weren’t there before.

Long found a dusty ring with two distinct, brilliant clusters of material circling within it at a distance of around 42 astronomical units from the star, or 42 times the distance between Earth and the Sun.

                Source: ANI