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News Release Archive:

News Release 762 of 954

January 17, 1996 08:30 AM (EST)

News Release Number: STScI-1996-02

Disk around Star May Be Warped by Unseen Planet

Background information useful for exploring this news release:

Science Background: the Dynamics of the Beta Pictoris Disk

Why Hasn't The Warp Been Detected Previously?

Though the Beta Pictoris Disk has been studied intensively for more than a decade the inner region of the disk is very hard to see with ground-based telescopes because of the glare from the central star. Also, the visible disk is faint because it consists of microscopic grains of ice and dust that shine only by reflecting light from the star. Hubble Space Telescope concentrates the star's light and produces an image that is ten times sharper than can be obtained from the ground under good conditions.

How Is The Lifetime of The Warp Determined?

Because the microscopic dust particles in the disk collide, in about a million years they either fall into the star or get broken up and blown out of the system by radiation pressure. Any warp in the visible disk will straighten out in even less time because of the same viscous processes. This means some continuous source of both particles and the warp must be in operation. The particles are probably the result of collisions within a belt of unseen larger comet-like objects which are tens of kilometers in diameter (like objects in the Kuiper belt around our own Solar System). In the absence of a planetary perturbation, gravity would straighten out any warp in this "Kupier belt" region within less than ten million years.

How Exactly Does a Planet Warp the Disk?

In 100 million years, a Jupiter-sized planet in a Jupiter-sized orbit would produce and maintain the warp Hubble sees. The Hubble results predict the planet's orbital plane is inclined by about three degrees to the outer disk. The comet-like bodies within the warped area precess, or wobble, around the planet's orbital plane and this leads to the inner disk being fattened and aligned with the planet's orbit. Material outside that radius has not time for its orbit to precess significantly, so appears in its original plane.

Why Is There a Central Clear Area in the Beta Pictoris Disk?

The central clear area, approximately the diameter of our Solar System, has long been suspected of harboring one or more planets which coalesced out of the disk. After planets form, they are expected to rapidly clear the visible disk in their vicinity. However, an alternative explanation was that the clear zone is the result of ices melting (sublimation).

What Was Known Previously about the Beta Pictoris Disk?

Discovered in 1983, the Beta Pictoris disk has long ben been considered a relic of planet formation. In 1775 philosopher Immanuel Kant proposed the nebular hypothesis of planet formation to explain the fact that the orbits of the planets almost lie in the same plane. He considered these coplanar orbits a "skeleton" of a primordial disk where the planets grew from smaller particles that stuck together to "snowball" into larger bodies — a process called agglomeration. (Hubble observations of the Orion star forming region find these disks are common in early stages of star formation.)

The disk about beta Pictoris was deduced from infrared observations obtained with NASA's Infrared Astronomical Satellite (IRAS). The discovery image was obtained by Brad Smith (University of Arizona) and Richard Terrile (JPL) in 1984 using a Charge Coupled Device (CCD) electronic camera with a coronagraph to block out the light from Beta Pictoris to reveal the faint disk. Such ground-based telescopic images of Beta Pictoris have revealed a nearly edge-on disk extending at least 100 billion miles from the star (1,000 times the distance between the Earth and Sun).

 
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