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A Circumstellar Disk Around β Pictoris

Smith, Bradford A., Terrile, Richard J.·1984·Science

Abstract

A circumstellar disk has been observed optically around the fourth-magnitude star β Pictoris. First detected in the infrared by the Infrared Astronomy Satellite last year, the disk is seen to extend to more than 400 astronomical units from the star, or more than twice the distance measured in the infrared by the Infrared Astronomy Satellite. The β Pictoris disk is presented to Earth almost edge-on and is composed of solid particles in nearly coplanar orbits. The observed change in surface brightness with distance from the star implies that the mass density of the disk falls off with approximately the third power of the radius. Because the circumstellar material is in the form of a highly flattened disk rather than a spherical shell, it is presumed to be associated with planet formation. It seems likely that the system is relatively young and that planet formation either is occurring now around β Pictoris or has recently been completed.

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Metadata

Authors
Smith, B. A., & Terrile, R. J.
Venue
Science
Published
1984-12-21
Volume
226
Issue
4681
Pages
1421-1424
ISSN
  • 0036-8075 (ISSN-L)
  • 1095-9203
OpenAlex
W2000146957
Cited by
734
References
0
FWCI
15.64
Type
journal article
Language
en
Open access
closed

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CoChat. (2026). Citation check: A Circumstellar Disk Around β Pictoris. https://app.cochat.ai/papers/10.1126/science.226.4681.1421
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Smith, B. A., & Terrile, R. J. (1984). A Circumstellar Disk Around β Pictoris. Science. https://doi.org/10.1126/science.226.4681.1421

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Semantic Scholar’s data is described in: Kinney, R., et al. (2023). The Semantic Scholar Open Data Platform. arXiv:2301.10140.