Beta Pictoris debris disk

Beta Pictoris debris disk

debris_disk

The Beta Pictoris debris disk is a vast, nearly edge-on ring of dust and rocky-icy debris around the young star Beta Pictoris, and the FIRST debris disk ever imaged around another star (1984). It is COLLISIONAL debris — comets and asteroids left from planet formation grinding one another to dust — warped and shepherded by the system's giant planets. Because we see it almost exactly edge-on, it appears as a thin bright line through the star; it is the archetype of a young planetary system caught in the act of forming.

Open in 3D viewSee Beta Pictoris debris disk in the live, interactive 3D map

Key facts

Type
Debris disk
Imaged
1984
the first ever
Orientation
Edge-on (~89°)

Science

Classification

Type
Collisional debris disk (seen nearly edge-on)
What it is
Dust and debris left from planet formation, replenished by colliding comets and asteroids — the first such disk ever imaged (1984)
Significance
The archetypal young planetary system — proof that other stars form planets, with giant planets found embedded in the disk itself

Structure

Extent
A vast disk detected out to hundreds of AU (traced to ~1,800 AU) · many times the size of the Solar System's planetary region
Orientation
Seen almost exactly edge-on from Earth (~89°) — a thin bright line · which is why it was the first disk to be imaged
Warps & belts
A warped inner disk and secondary belts — signatures of the system's giant planets gravitationally sculpting the debris

How we know

Note
The disk is real and directly imaged — the first debris disk ever pictured around another star. It is shown edge-on, its true orientation, as a soft dust band; the fine warps and belts are modelled/illustrative, not a photograph, and the giant planets embedded in it are shown at their real measured orbits.

Discovery & history

Method
Infrared excess (space telescope)
Name
Named for its host star, Beta Pictoris; the disk has no separate proper name.

First photographed in 1984 by Bradford Smith and Richard Terrile after IRAS detected the star's infrared excess — the disk that proved other stars really do form planetary systems, and where Beta Pic b was later found embedded.

Images

Images from open archives · credit shown per image