Archivo de imágenes de Hubble
Sombra en el disco de TW Hydrae
These images, taken a year apart by NASA's Hubble Space Telescope, reveal a shadow moving counterclockwise around a gas-and-dust disk encircling the young star TW Hydrae.The two images at the top, taken by the Space Telescope Imaging Spectrograph, show an uneven brightness across...
- Fecha
- Jan 1, 2017
- Misión
- Hubble Space Telescope
- ID de archivo
- hubblesite-images-2017-03-3972-image
These images, taken a year apart by NASA's Hubble Space Telescope, reveal a shadow moving counterclockwise around a gas-and-dust disk encircling the young star TW Hydrae.
The two images at the top, taken by the Space Telescope Imaging Spectrograph, show an uneven brightness across the disk.
Through enhanced image processing (images at bottom), the darkening becomes even more apparent. These enhanced images allowed astronomers to determine the reason for the changes in brightness.
The dimmer areas of the disk, at top left, are caused by a shadow spreading across the outer disk. The dotted lines approximate the shadow's coverage. The long arrows show how far the shadow has moved in a year (from 2015-2016), which is roughly 20 degrees.
Based on Hubble archival data, astronomers determined that the shadow completes a rotation around the central star every 16 years. They know the feature is a shadow because dust and gas in the disk do not orbit the star nearly that quickly. So, the feature must not be part of the physical disk.
The shadow may be caused by the gravitational effect of an unseen planet orbiting close to the star. The planet pulls up material from the main disk, creating a warped inner disk. The twisted disk blocks light from the star and casts a shadow onto the disk's outer region.
Credits
NASA, ESA, and J. Debes (STScI)Detalles de la imagen
| About The Object | |
|---|---|
| Object Name | TW Hydrae |
| Object Description | T Tauri Star |
| R.A. Position | 11h 01m 51.91s |
| Dec. Position | -34º 42’ 17.0” |
| Constellation | Hydra |
| Distance | About 180 light-years (54 parsecs). The images are approximately 6 arcseconds, or roughly 400 AU, wide. |
| About The Data | |
| Data Description | Datasets used for these results are from the HST proposal 13753, John Debes (STScI) P.I. and lead author. |
| Instrument | HST>STIS/CCD |
| Exposure Dates | May 2015, March 2016 |
| Filters | 50CCD |
| About The Image | |
| Color Info | The images were acquired by HST’s STIS CCD instrument using the 50CCD (clear imaging) filter. Color was applied using a colormap assigning a different color to each brightness value. |
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Fuente
La imagen y el material de referencia se acreditan al archivo oficial de la misión enlazado a continuación.
Ver en NASA.gov