Back
Image: Hubble Servicing Mission 4 Early Release Observations
ABOUT THIS IMAGE:
These four images are among the first observations made by the new Wide Field Camera 3 aboard the upgraded NASA Hubble Space Telescope.
The image at top left shows NGC 6302, a butterfly-shaped nebula surrounding a dying star. At top right is a picture of a clash among members of a galactic grouping called Stephan's Quintet. The image at bottom left gives viewers a panoramic portrait of a colorful assortment of 100,000 stars residing in the crowded core of Omega Centauri, a giant globular cluster. At bottom right, an eerie pillar of star birth in the Carina Nebula rises from a sea of greenish-colored clouds.
Object Names: NGC 6302, Stephan's Quintet, Omega Centauri, Jet in Carina
Image Type: Astronomical
Credit: NASA, ESA, and the Hubble SM4 ERO Team
Technical facts about this image:
About NGC 6302
 |
| Object Name: |
NGC 6302 (Butterfly Nebula, Bug Nebula) |
| Object Description: |
Planetary Nebula |
| Position (J2000): |
R.A. 17h 13m 43s.3
Dec. -37° 06' 10" |
| Distance: |
3,800 light-years (1,200 parsecs) |
| Constellation: |
Scorpius |
| Data Description: |
The Hubble images were created from data from proposal 11504: K. Noll and H. Bond (STScI) and B. Balick (University of Washington). |
| Instrument: |
WFC3/UVIS |
| Exposure Date(s): |
July 27, 2009 |
| Exposure Time: |
1.5 hours |
| Filters: |
F373N ([O II]), F469N (He II), F502N ([O III]), F656N (H-alpha), F658N ([N II]), and F673N ([S II]) |
|
About Jet in Carina
 |
| Object Name: |
Jet in Carina |
| Object Description: |
Stellar Jet/Young Stellar Object |
| Position (J2000): |
R.A. 10h 43m 51s.30
Dec. -59° 55' 21".0 |
| Constellation: |
Carina |
| Distance: |
7,500 light-years (2,300 parsecs) |
| Dimensions: |
This image is 3 arcminutes (6.6 light-years or 2.0 parsecs) wide. |
| Data Description: |
The Hubble images were created from data from proposal 11501: K. Noll (STScI), C. Proffitt (STScI/CSC), D. Leckrone and M. Niedner (NASA/GSFC), and M. Livio and Z. Levay (STScI). |
| Instrument: |
WFC3/IR and WFC3/UVIS |
| Exposure Date(s): |
July 24-30, 2009 |
| Exposure Time: |
8.4 hours |
| Filters: |
WFC3/IR: F126N ([Fe II]) and F164N ([Fe II]) WFC3/UVIS: F280N (Mg II), F502N ([O III]), F656N (H-alpha), and F673N ([S II]) |
|
About Omega Centauri
 |
| Object Name: |
Omega Centauri (NGC 5139) |
| Object Description: |
Globular Star Cluster |
| Position (J2000): |
R.A. 13h 26m 45s.9
Dec. -47° 28' 37" |
| Constellation: |
Centaurus |
| Distance: |
16,000 light-years or 4,800 parsecs |
| Data Description: |
The Hubble images were created from data from the calibration proposal 11452: E. Sabbi, J. Kim Quijano, and L. Dressel (STScI). |
| Instrument: |
WFC3/UVIS |
| Exposure Date(s): |
July 15, 2009 |
| Exposure Time: |
2.7 hours |
| Filters: |
F225W (U), F275W (U), F336W (U), F438W (B), F606W (V), and F814W (I) |
|
About Stephan's Quintet
 |
| Object Name: |
Stephan's Quintet (HCG 92) |
| Object Description: |
Interacting Galaxy Group |
| Position (J2000): |
R.A. 22h 35m 57s.51
Dec. +33° 57' 35".68 |
| Constellation: |
Pegasus |
| Distance: |
Stephan's Quintet is 290 million light-years (90 million parsecs) away. NGC 7320, superposed in the foreground, is 40 million light-years (12 million parsecs) away. |
| Data Description: |
The Hubble images were created from data from proposal 11502: K. Noll and M. Livio (STScI), D. Leckrone and M. Niedner (NASA/GSFC), and Z. Levay and M. Mutchler (STScI). |
| Instrument: |
WFC3/IR and WFC3/UVIS |
| Exposure Date(s): |
July/August 2009 |
| Exposure Time: |
17 hours |
| Filters: |
WFC3/IR: F140W (J-H)
WFC3/UVIS: F438W (B), F606W (V), F657N (H-alpha + [N II]), F665N (H-alpha + [N II]), and F814W (I) |
|
The above montage includes these images:
NGC 6302
Image Type: Astronomical
Stephan's Quintet
Image Type: Astronomical
Omega Centauri
Image Type: Astronomical
Jet in Carina
Image Type: Astronomical
All images from this news release:
To access available information and downloadable versions of images in this news release, click on any of the images below: