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ESO 42/08 - Associated Images
21 November 2008
For Immediate Release
Beta Pictoris planet finally imaged?
ESO PR Photo 42a/08
Beta Pictoris as seen in infrared light
[Preview - JPEG: 402 x 400 pix - 46k]
[Normal - JPEG: 803 x 800 pix - 100k]
[Full Res - JPEG: 990 x 985 pix - 136k]
[Full Res - TIFF: 990 x 985 pix - 761k]
This composite image represents the close environment of Beta Pictoris as seen in near infrared light. This very faint environment is revealed after a very careful subtraction of the much brighter stellar halo. The outer part of the image shows the reflected light on the dust disc, as observed in 1996 with the ADONIS instrument on ESO's 3.6 m telescope; the inner part is the innermost part of the system, as seen at 3.6 microns with NACO on the Very Large Telescope. The newly detected source is more than 1000 times fainter than Beta Pictoris, aligned with the disc, at a projected distance of 8 times the Earth-Sun distance. This corresponds to 0.44 arcsecond on the sky, or the angle sustained by a one Euro coin seen at a distance of about 10 kilometres. Because the planet is still very young, it is still very hot, with a temperature around 1200 degrees Celsius. Both parts of the image were obtained on ESO telescopes equipped with adaptive optics.
Credit: ESO/A.-M. Lagrange et al.
ESO PR Photo 42b/08
Beta Pictoris as seen in infrared light - annotated
[Preview - JPEG: 402 x 400 pix - 51k]
[Normal - JPEG: 803 x 800 pix - 114k]
[Full Res - JPEG: 990 x 985 pix - 153k]
[Full Res - TIFF: 990 x 985 pix - 794k]
This composite image represents the close environment of Beta Pictoris as seen in near infrared light. This very faint environment is revealed after a very careful subtraction of the much brighter stellar halo. The outer part of the image shows the reflected light on the dust disc, as observed in 1996 with the ADONIS instrument on ESO's 3.6 m telescope; the inner part is the innermost part of the system, as seen at 3.6 microns with NACO on the Very Large Telescope. The newly detected source is more than 1000 times fainter than Beta Pictoris, aligned with the disc, at a projected distance of 8 times the Earth-Sun distance. Both parts of the image were obtained on ESO telescopes equipped with adaptive optics.
Credit: ESO/A.-M. Lagrange et al.
ESO PR Photo 42c/08
Candidate planetary systems imaged
[Preview - JPEG: 790 x 400 pix - 62k]
[Normal - JPEG: 1580 x 800 pix - 122k]
[Full Res - JPEG: 1519 x 3000 pix - 283k]
[Full Res - TIFF: 1519 x 3000 pix - 276k]
This diagramme compares the various candidate planetary systems that have been imaged for now, with our Solar System. Indicated are the star and the position of the imaged candidate planets. The probable planet around Beta Pictoris is the closest to its host star of all extra-solar planets yet imaged, and is comparable to Saturn as far as its distance is concerned. The scale is the distance between the Earth and the Sun.
A list of all candidate exoplanets directly imaged can be found at
http://exoplanet.eu/catalog-imaging.php
Credit: ESO


