Binary brown dwarf Kelu-1

These NASA/ESA Hubble Space Telescope images of the binary brown dwarf Kelu-1 trace the orbital motion of the two stars over a seven-year span as photographed by the Near Infrared Camera and Multi-Object Spectrometer (NICMOS) on Hubble.

In 1998, the "stars" were too close together to be resolved by Hubble. By 2005, they had moved apart to a separation of 835 million kilometres. The projected maximum separation is 885 million kilometres.

Binary systems allow astronomers to estimate the mass of companion objects. The brown dwarfs are 61 and 50 times the mass of Jupiter. They are therefore too small to burn as stars, but too large to have formed as planets. Based on the total estimated mass of the system, astronomers suspect there is a third brown dwarf member that has not yet been resolved.

Credit:

NASA, ESA and M. Stumpf (Max-Planck-Institute for Astronomy)

About the Image

NASA press release
NASA caption
Id:opo0901a
Type:Collage
Release date:5 January 2009, 18:20
Size:3000 x 2400 px

About the Object

Name:Kelu-1
Type:• Milky Way : Star : Type : Brown Dwarf
• Milky Way : Star : Grouping : Binary
• X - Stars Images/Videos
Distance:60 light years

Colours & filters

BandTelescope
Infrared
Near-IR
Hubble Space Telescope
NICMOS

Image Formats

Large JPEG
307.2 KB
Screensize JPEG
81.8 KB

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