Hubble image of variable star RS Puppis
This Hubble image shows RS Puppis, a type of variable star known as a Cepheid variable. As variable stars go, Cepheids have comparatively long periods — RS Puppis, for example, varies in brightness by almost a factor of five every 40 or so days.
RS Puppis is unusual; this variable star is shrouded by thick, dark clouds of dust enabling a phenomenon known as a light echo to be shown with stunning clarity.
These Hubble observations show the ethereal object embedded in its dusty environment, set against a dark sky filled with background galaxies.
Credit:NASA, ESA, and the Hubble Heritage Team (STScI/AURA)-Hubble/Europe Collaboration
Acknowledgment: H. Bond (STScI and Penn State University)
About the Image
Id: | heic1323a |
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Type: | Observation |
Release date: | 17 December 2013, 16:00 |
Related releases: | heic1323 |
Related announcements: | ann1908 |
Related science announcements: | sci19006, sci19002, sci15008 |
Size: | 3981 x 3910 px |
About the Object
Name: | RS Puppis |
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Type: | Milky Way : Star : Type : Variable : Pulsating Milky Way : Nebula : Appearance : Reflection : Light Echo |
Distance: | 6500 light years |
Constellation: | Puppis |
Category: | Nebulae Stars |
Coordinates
Position (RA): | 8 13 4.20 |
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Position (Dec): | -34° 34' 42.73" |
Field of view: | 3.32 x 3.26 arcminutes |
Orientation: | North is 91.0° right of vertical |
Colours & filters
Band | Wavelength | Telescope |
---|---|---|
Optical B | 435 nm |
Hubble Space Telescope
ACS |
Optical V | 606 nm |
Hubble Space Telescope
ACS |