proto-planetary disc – Astronomy Now

Habitable worlds orbiting dwarf stars may not be commonplace after all

9 January 2019 Astronomy Now

Observations by the Hubble Space Telescope and ESO’s Very Large Telescope indicate processes that may limit the habitability of planets orbiting dwarf stars.

Baby star throws a fit, erupts with titanic flare

28 December 2018 Astronomy Now

Astronomers have observed a titanic flare on a young star that was 10,000 times more powerful than any outburst ever recorded from Earth’s Sun, possibly influencing the eventual development of planets.

Astronomers catch new planet in the process of forming

2 July 2018 Astronomy Now

Astronomers have managed to spot a new planet in the process of forming in a dusty disk surrounding a hot young star. It is the first definitive observation of its kind, opening a new window in exoplanet research.

Understanding stellar adolescence through T-Tauri stars

13 June 2016 Astronomy Now

A newborn star typically goes through four stages of adolescence. It begins life as a protostar, accreting material and developing a proto-planetary disc. Slowly, stellar winds and radiation blow away the surrounding shell of gas and dust. Next, when the surrounding envelope has cleared, is called the T-Tauri phase. Finally, accretion stops and the source’s radiation comes from the star’s photosphere.

The minimum mass of a proto-solar system disc

20 October 2015 Astronomy Now

Astronomers studying the birth of planetary systems in the young (about 2-3 million years old) star forming region IC348 in Perseus as seen by the infrared cameras onboard the Spitzer Space Telescope have found thirteen stars in this complex with detectable discs, none of which is as massive as our early solar system’s disc.

Astronomers peer into the ‘amniotic sac’ of a planet-hosting star

14 September 2015 Astronomy Now

An international team of astronomers have successfully peered through the ‘amniotic sac’ of an embryonic star to observe the innermost region of a burgeoning solar system for the first time. The magnitude +6.8 star, which is called HD 100546 or KR Muscae, lies 325 light-years away in the far southern constellation Musca.