Young Planets Bite the Dust

These orange swirls of dust are snapshots from the largest collection of sharp, detailed images of dusty debris disks around young stars - published this week by an international group of astronomers.

The images - captured by the 8-meter Gemini South telescope using the Gemini Planet Imager - illustrate the variety of shapes and sizes that stellar systems can take during their infancy. Unexpectedly, the majority of these systems display evidence of planet formation.

These remarkable portraits of dusty disks are a selection from 26 new images of debris disks obtained by the Gemini Planet Imager (GPI) at the international Gemini Observatory, a Program of NSF's NOIRLab. These images highlight the diversity of shapes and sizes that these disks can take and show the outer reaches of exoplanetary systems in their formative years.

The young stars imaged, which range from tens of millions to a few hundred million years old, are at the ideal age to settle down and raise planets. The forming planets sculpt the dust disk and leave behind gaps and warps that are indirect clues to their existence and motion.

While debris disks have been imaged before, this new cohort of 26 disks represents one of the largest samples to be imaged with highly uniform data quality. This enables detailed comparison of the observations, a unique breakthrough in debris disk surveys.

Thirteen of the disks form a perfect natural laboratory, all belonging to the Scorpius-Centaurus stellar association, roughly 400 light-years from Earth. The group of stars, which were born in the same region at roughly the same time, enables astronomers to compare the architectures of a variety of young planetary systems developing under different conditions.

GPI was able to capture these dusty disks with the help of some ingenious astronomical engineering. GPI is sensitive to the polarization of light, allowing it to distinguish dust-scattered light, which is polarized, from the unpolarized light emanating from the stars.

This gives GPI the impressive ability to improve the contrast of images and capture disks that are 10 million times fainter than their parent stars. Measuring polarization is only one of GPI's tricks, however - the instrument also exploits a coronagraph and adaptive optics to get the most from its observations.

GPI's precision is in large part due to its perch on the 8-meter Gemini South telescope on Cerro Pachon in Chile. The dry conditions, high altitude, and dark skies are perfect for cutting-edge astronomical research. By combining this exquisite location with some engineering ingenuity, GPI is able to capture images as sharp as those from the Hubble Space Telescope - and detect objects up to three times closer to the host stars.

GPI's first-rate observing abilities enabled this work, part of the Gemini Planet Imager Exoplanet Survey (GPIES), a 4-year search for light emitted by giant gas planets orbiting more than 500 of the youngest stars near the Sun.

As well as doubling the number of debris disks imaged at this high resolution, the survey uncovered six giant exoplanets and four brown dwarfs. Surveys such as GPIES are a perfect way to screen targets for the next generation of space- and ground-based telescopes.

"The Gemini instrument program continues to provide unique science opportunities. This combination of GPI mounted upon a large ground-based telescope is delivering exciting new details about the process of how planets form," said Martin Still, NSF Program Manager for the Gemini Observatory partnership.

The GPIES survey concluded in 2019, but the investment and technical capability of the Gemini Planet Imager will continue with an upgrade to GPI's hardware to improve its resolution and sensitivity.

The new "GPI 2.0," is slated for a future installation at Gemini North atop Maunakea in Hawaii, where it will search the less-observed northern hemisphere skies for more exoplanets and debris disks. GPI 2.0 will also continue the work of scouting out targets for the next generation of exoplanet missions, setting the scene for new insights into the mystery of planet formation.

Research Report: "Debris Disk Results from the Gemini Planet Imager Exoplanet Survey's Polarimetric Imaging Campaign"

Related Links
International Gemini Observatory
Lands Beyond Beyond - extra solar planets - news and science
Life Beyond Earth

Tweet

Thanks for being there;
We need your help. The SpaceDaily news network continues to grow but revenues have never been harder to maintain.

With the rise of Ad Blockers, and Facebook - our traditional revenue sources via quality network advertising continues to decline. And unlike so many other news sites, we don't have a paywall - with those annoying usernames and passwords.

Our news coverage takes time and effort to publish 365 days a year.

If you find our news sites informative and useful then please consider becoming a regular supporter or for now make a one off contribution.

SpaceDaily Monthly Supporter
$5+ Billed Monthly

paypal only

SpaceDaily Contributor
$5 Billed Once

credit card or paypal

Are Planets with Oceans Common in the Galaxy? It's Likely, NASA Scientists Find
Greenbelt MD (SPX) Jun 19, 2020
Several years ago, planetary scientist Lynnae Quick began to wonder whether any of the more than 4,000 known exoplanets, or planets beyond our solar system, might resemble some of the watery moons around Jupiter and Saturn. Though some of these moons don't have atmospheres and are covered in ice, they are still among the top targets in NASA's search for life beyond Earth. Saturn's moon Enceladus and Jupiter's moon Europa, which scientists classify as "ocean worlds," are good examples. "Plumes of w ... read more