Long before medieval alchemists dreamed of transmuting base metals to gold [
http://antwrp.gsfc.
], stellar furnaces in this massive cluster of galaxies - cataloged as RDCS 1252.9-2927 - had transformed light elements into heavy ones [
http://helios.gsfc.
]. In the false-color composite image [
http://chandra.harv
] individual cluster galaxies can be seen at optical and near-infrared wavelengths, shown in red, yellow, and green colors. X-ray [
http://chandra.harv
] data (in purple) reveal the hot intracluster gas [
http://chandra.harv
galaxy_clusters.html ], enriched in heavy elements. Attracting the attention of astronomers using the orbiting Chandra [
http://chandra.harv
] and XMM-Newton [
http://sci.esa.int/
index.cfm?fareaid=23 ] x-ray telescopes, as well as the Hubble Space Telescope [
http://hubblesite.o
releases/2004/01/ ] and ground based VLT [
http://www.eso.org/
], the galaxy cluster lies nearly 9 billion light-years away [
http://www.faqs.org
part8/section-14.htm l ] ... and so existed at a time when the Universe was less than 5 billion years old. A measured mass of more than 200 trillion [
http://www.unc.edu/
large.html ] Suns makes this galaxy cluster the most massive object ever found when the Universe was so young. The cluster elemental abundances [
http://arxiv.org/ab
] are consistent with the idea that most heavy elements were synthesized early on by massive stars, but current theories suggest that such a massive cluster should be rare in the early Universe [
http://www.us-gemin
announcements/press/ 2004-1.html ].
Explanation
Long before medieval alchemists dreamed of transmuting base metals to gold [
http://antwrp.gsfc.
], stellar furnaces in this massive cluster of galaxies - cataloged as RDCS 1252.9-2927 - had transformed light elements into heavy ones [
http://helios.gsfc.
]. In the false-color composite image [
http://chandra.harv
] individual cluster galaxies can be seen at optical and near-infrared wavelengths, shown in red, yellow, and green colors. X-ray [
http://chandra.harv
] data (in purple) reveal the hot intracluster gas [
http://chandra.harv
galaxy_clusters.html ], enriched in heavy elements. Attracting the attention of astronomers using the orbiting Chandra [
http://chandra.harv
] and XMM-Newton [
http://sci.esa.int/
index.cfm?fareaid=23 ] x-ray telescopes, as well as the Hubble Space Telescope [
http://hubblesite.o
releases/2004/01/ ] and ground based VLT [
http://www.eso.org/
], the galaxy cluster lies nearly 9 billion light-years away [
http://www.faqs.org
part8/section-14.htm l ] ... and so existed at a time when the Universe was less than 5 billion years old. A measured mass of more than 200 trillion [
http://www.unc.edu/
large.html ] Suns makes this galaxy cluster the most massive object ever found when the Universe was so young. The cluster elemental abundances [
http://arxiv.org/ab
] are consistent with the idea that most heavy elements were synthesized early on by massive stars, but current theories suggest that such a massive cluster should be rare in the early Universe [
http://www.us-gemin
announcements/press/ 2004-1.html ].
Explanation