దస్త్రం:Sn2006gy collapse ill.jpg

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అసలు దస్త్రం ‎(3,870 × 2,400 పిక్సెళ్ళు, ఫైలు పరిమాణం: 795 KB, MIME రకం: image/jpeg)

వివరణ Original caption: "This illustration explains the process that astronomers think triggered the explosion in SN 2006gy. When a star is very massive, its core can produce so much gamma-ray light that some of the energy from the radiation is converted into particle and anti-particle pairs. The resulting drop in energy causes the star to collapse under its own huge gravity. After this violent collapse, runaway thermonuclear reactions (not shown here) ensue and the star explodes, spewing the remains into space."
తేదీ అజ్ఞాత తేదీ
Unknown date
మూలం http://chandra.harvard.edu/photo/2007/sn2006gy/more.html, specifically http://chandra.harvard.edu/photo/2007/sn2006gy/sn2006gy_ill.tif
కర్త NASA/CXC/M. Weiss
అనుమతి
(ఈ దస్త్రాన్ని పునర్వినియోగించుకోవడం)

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ఇతర కూర్పులు
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చిత్రణ

ఫైలు చరితం

తేదీ/సమయం ను నొక్కి ఆ సమయాన ఫైలు ఎలా ఉండేదో చూడవచ్చు.

తేదీ/సమయంనఖచిత్రంకొలతలువాడుకరివ్యాఖ్య
ప్రస్తుత23:12, 9 మే 200723:12, 9 మే 2007 నాటి కూర్పు నఖచిత్రం3,870 × 2,400 (795 KB)Tom{{Information |Description=Original caption: "This illustration explains the process that astronomers think triggered the explosion in SN 2006gy. When a star is very massive, its core can produce so much gamma-ray light that some of the energy from th

కింది పేజీలలో ఈ ఫైలుకు లింకులు ఉన్నాయి:

సార్వత్రిక ఫైలు వాడుక

ఈ దస్త్రాన్ని ఈ క్రింది ఇతర వికీలు ఉపయోగిస్తున్నాయి:

మెటాడేటా

ఈ ఫైలులో అదనపు సమాచారం ఉంది, బహుశా దీన్ని సృష్టించడానికి లేదా సాంఖ్యీకరించడానికి వాడిన డిజిటల్ కేమెరా లేదా స్కానర్ ఆ సమాచారాన్ని చేర్చివుండవచ్చు. ఈ ఫైలును అసలు స్థితి నుండి మారిస్తే, ఆ మారిన ఫైలులో కొన్ని వివరాలు పూర్తిగా ప్రతిఫలించకపోవచ్చు.

"https://te.wikipedia.org/wiki/దస్త్రం:Sn2006gy_collapse_ill.jpg" నుండి వెలికితీశారు