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More Images of Galaxy Clusters & the Hubble Constant
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Chandra X-ray Image of CL 0016+1609
A critically important number that sets the expansion rate of the Universe, the so-called Hubble constant, has been independently determined using NASA's Chandra X-ray Observatory. This new value matches recent measurements using other methods and extends their validity to greater distances and thus allows astronomers to probe earlier epochs in the evolution of the Universe. These images show six of the 38 galaxy clusters that scientists observed with Chandra.
| Fast Facts for CL 0016+1609: |
| Credit |
NASA/CXC/MSFC/M.Bonamente et al. |
| Scale |
Image is 4.4 arcmin across |
| Coordinates (J2000) |
RA 00h 18m 33.50s | Dec +16º 26' 12.50" |
| Constellation |
Pisces |
| Observation Date |
18 Aug 2000
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| Observation Time |
19 hours |
| Obs. ID |
520 |
| Distance Estimate |
About 4.5 billion (z=0.54) light years |
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Chandra X-ray Image of Abell 665
| Fast Facts for Abell 665: |
| Credit |
NASA/CXC/MSFC/M.Bonamente et al. |
| Scale |
Image is 5.6 arcmin across |
| Coordinates (J2000) |
RA 08h 30m 58.10s | Dec +65º 50' 51.60" |
| Constellation |
Ursa Major |
| Observation Date |
28 Dec 2002
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| Observation Time |
8 hours |
| Obs. ID |
3586 |
| Distance Estimate |
About 2.2 billion (z=0.18) light years |
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Chandra X-ray Image of MACS J1149.5+223
| Fast Facts for MACS J1149.5+223: |
| Credit |
NASA/CXC/MSFC/M.Bonamente et al. |
| Scale |
Image is 4.2 arcmin across |
| Coordinates (J2000) |
RA 11h 49m 35.50s | Dec +22º 24' 02.30" |
| Constellation |
Leo Minor |
| Observation Date |
01 Jun 2001, 07 Feb 2003
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| Observation Time |
11 hours |
| Obs. ID |
1656, 3589 |
| Distance Estimate |
About 2.6 billion (z=0.54) light years |
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Chandra X-ray Image of CL J1226.9+3332
| Fast Facts for CL J1226.9+3332: |
| Credit |
NASA/CXC/MSFC/M.Bonamente et al. |
| Scale |
Image is 4.4 arcmin across |
| Coordinates (J2000) |
RA 12h 26m 57.90s | Dec +33º 32' 47.40" |
| Constellation |
Canes Venatici |
| Observation Date |
27 Jan 2003, 31 Jul 2000
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| Observation Time |
12 hours |
| Obs. ID |
3180, 932 |
| Distance Estimate |
About 3.5 billion (z=0.89) light years |
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Chandra X-ray Image of Abell 1689
| Fast Facts for Abell 1689: |
| Credit |
NASA/CXC/MSFC/M.Bonamente et al. |
| Scale |
Image is 8.1 arcmin across |
| Coordinates (J2000) |
RA 13h 11m 29.50s | Dec -01º 20' 28.20" |
| Constellation |
Virgo |
| Observation Date |
07 Jan 2001, 15 Apr 2000
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| Observation Time |
6 hours |
| Obs. ID |
1663, 540 |
| Distance Estimate |
About 2.1 billion (z=0.18) light years |
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Chandra X-ray Image of Abell 1914
| Fast Facts for Abell 1914: |
| Credit |
NASA/CXC/MSFC/M.Bonamente et al. |
| Scale |
Image is 7.6 arcmin across |
| Coordinates (J2000) |
RA 14h 26m 00.80s | Dec +37º 49' 35.70" |
| Constellation |
Boötes |
| Observation Date |
03 Sep 2003, 21 Nov 1999
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| Observation Time |
7 hours |
| Obs. ID |
3593, 542 |
| Distance Estimate |
About 1.4 billion (z=0.17) light years |
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Illustration of Sunyaev-Zeldovich Effect
The astronomers in this study used a phenomenon known as the Sunyaev-Zeldovich effect, where photons in the cosmic microwave background interact with electrons in the hot gas that pervades the enormous galaxy clusters. The photons acquire energy from this interaction, which distorts the signal from the microwave background in the direction of the clusters. This illustration depicts this concept graphically by the broad bright beams emanating from the cluster.
(Illustration: NASA/CXC/M.Weiss)
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| 8 |
| CL 0016+1609 with Scale Bar
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