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 |
|---|---|
| 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 |
|---|---|
| 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 |
|---|---|
| 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 |

