Hubble image archive
Hubble Catches a Dusty Moth
These near-infrared images, taken with the Near-Infrared Camera and Multi-Object Spectrometer (NICMOS) aboard NASA's Hubble Space Telescope, show the wing- shaped dust disk surrounding the young, nearby star HD 61005. Astronomers have dubbed the star system "The Moth" because the...
- Date
- Jan 1, 2008
- Mission
- Hubble Space Telescope
- Archive ID
- hubblesite-images-2008-01-2229-image
These near-infrared images, taken with the Near-Infrared Camera and Multi-Object Spectrometer (NICMOS) aboard NASA's Hubble Space Telescope, show the wing- shaped dust disk surrounding the young, nearby star HD 61005. Astronomers have dubbed the star system "The Moth" because the dust disk resembles the wings of the flying insect.
The Moth's wingspan extends about 22 billion miles from the star. The black disk in the center of the images represents the coronagraphic hole in the NICMOS camera that blocks most of the starlight so that astronomers can see details in the surrounding dust disk.
HD 61005 is about 100 million years old. Dust disks around stars of The Moth's age are typically flat structures where planets can form. These Hubble images show that some dust disks have some surprising shapes. HD 61005 appears to be plowing through a local patch of higher-density gas in the interstellar medium, causing material in the HD 61005's disk to be swept behind the star.
HD 61005 resides 100 light-years from Earth. NICMOS took these images in 2005 and 2006.
Credits
NASA, D. Hines (Space Science Institute, New Mexico Office in Corrales, New Mexico), and G. Schneider (University of Arizona)Image Details
| About The Object | |
|---|---|
| Object Name | HD 61005, The Moth |
| Object Description | Star with Circumstellar Structure |
| R.A. Position | 07h 35m 47.45s |
| Dec. Position | -32° 12' 14.04" |
| Constellation | Puppis |
| Distance | 100 light-years or 31 parsecs |
| About The Data | |
| Data Description | HST Proposal: D. Hines (Space Science Institute, New Mexico Office in Corrales, New Mexico). The science team comprises: D. Hines (Space Science Institute, New Mexico Office in Corrales, New Mexico), G. Schneider (University of Arizona) , D. Hollenbach (NASA Ames), E. Mamajek (Harvard-Smithsonian Center for Astrophysics), L. Hillenbrand (California Institute of Technology), S. Metchev (University of California, Los Angeles), M. Meyer (University of Arizona), J . Carpenter (California Institute of Technology), A. Moro-Martin (Princeton University), M. Silverstone (Eureka Scientific, Cary, NC), J. Serena Kim (University of Arizona), and T. Henning, J. Bouwman, and S. Wolf (Max Planck Institute for Astronomy, Heidelberg, Germany). |
| Instrument | HST>NICMOS |
| Exposure Dates | November 20, 2005; June 18, 2006, Exposure Time: 1.3 hours |
| Filters | F110W (J-band) |
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Image and source material are credited to the official mission archive linked below.
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