These images represent views of Kepler's supernova remnant taken in X-rays, visible light, and infrared radiation.
Each top panel shows the entire remnant. Each color in this image represents a different region of the electromagnetic spectrum, from X-rays to infrared light. The X-ray and infrared data cannot be seen with the human eye. Astronomers have color-coded those data so they can be seen in these images.
The bottom panels are close-up views of the remnant. The region seen in these images is outlined in the top row of pictures. In the bottom, center image, Hubble sees fine details in the brightest, densest areas of gas.
The images indicate that the bubble of gas that makes up the supernova remnant appears different in various types of light. Chandra reveals the hottest gas [colored blue and colored green], which radiates in X-rays. The blue color represents the higher-energy gas; the green, the lower-energy gas. Hubble shows the brightest, densest gas [colored yellow], which appears in visible light. Spitzer unveils heated dust [colored red], which radiates in infrared light.
Credits
NASA, ESA, R. Sankrit and W. Blair (Johns Hopkins University)| About The Object | |
|---|---|
| Object Name | Kepler's Supernova Remnant, SN 1604, V 843 Ophiuchi, G004.5+06.8 |
| Object Description | Supernova Remnant |
| R.A. Position | 17h 30m 40.79s |
| Dec. Position | -21° 29' 11.0" |
| Constellation | Ophiuchus |
| Distance | 13,000 light-years (4,000 parsecs) |
| About The Data | |
| Data Description | Chandra Data This image was created from Chandra observations from proposal 01500022: S. Holt (F.W. Olin College of Engineering), U. Hwang, R. Petre, and M. Corcoran (GSFC), E. Gotthelf (Columbia Astrophysics Lab), G. Allen (Massachusetts Inst. of Tech.), J. Keohane (North Carolina). The science team using this data is: R. Sankrit and W. Blair (Johns Hopkins Univ.), T. DeLaney (U. Minnesota and Harvard-Smithsonian/Center for Astrophysics), L. Rudnick and J. A. Ennis (U. Minnesota), I. Harrus (Goddard Space Flight Center). Hubble Data This image was created from Hubble observations from proposal : R. Sankrit and W. Blair (Johns Hopkins Univ.), L. Rudnick (U. Minnesota), T. DeLaney (U. Minnesota and Harvard-Smithsonian/Center for Astrophysics), I. Harrus (Goddard Space Flight Center). Spitzer Data This image was created from Spitzer observations from proposal 3413: W. Blair, R. Sankrit, and P. Ghavamian (Johns Hopkins Univ.), K. Borkowski and S. Reynolds (North Carolina State Univ.), and K. Long (Space Telescope Science Inst.). |
| Instrument | CXO>ACIS-S; HST>ACS/WFC and HST>WFPC2; SST>MIPS and SST>IRAC |
| Exposure Dates | June 30, 2000 (CXO), August 28-29, 2003 and May 26, 2004 (HST), August 25, 2004 and September 3, 2004 (SST) |
| Filters | CXO: 0.3-6 keV HST: F502N ([O III]), F550M (V), F658N (Halpha+[N II]), F660N ([N II]), and F673N ([S II]) SST: MIPS 24 and 70 micron; IRAC 4.5 and 8 micron |
| About The Object | |
|---|---|
| Object Name | A name or catalog number that astronomers use to identify an astronomical object. |
| Object Description | The type of astronomical object. |
| R.A. Position | Right ascension – analogous to longitude – is one component of an object's position. |
| Dec. Position | Declination – analogous to latitude – is one component of an object's position. |
| Constellation | One of 88 recognized regions of the celestial sphere in which the object appears. |
| Distance | The physical distance from Earth to the astronomical object. Distances within our solar system are usually measured in Astronomical Units (AU). Distances between stars are usually measured in light-years. Interstellar distances can also be measured in parsecs. |
| Dimensions | The physical size of the object or the apparent angle it subtends on the sky. |
| About The Data | |
| Data Description |
|
| Instrument | The science instrument used to produce the data. |
| Exposure Dates | The date(s) that the telescope made its observations and the total exposure time. |
| Filters | The camera filters that were used in the science observations. |
| About The Image | |
| Image Credit | The primary individuals and institutions responsible for the content. |
| Publication Date | The date and time the release content became public. |
| Color Info | A brief description of the methods used to convert telescope data into the color image being presented. |
| Orientation | The rotation of the image on the sky with respect to the north pole of the celestial sphere. |
