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X-rays from comets - a surprising discovery

<!--HTML-->Comets are kilometre-size aggregates of ice and dust, which remained from the formation of the solar system. It was not obvious to expect X-ray emission from such objects. Nevertheless, when comet Hyakutake (C/1996 B2) was observed with the ROSAT X-ray satellite during its close app...

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Autor principal: CERN. Geneva
Lenguaje:eng
Publicado: CERN 2000
Materias:
Acceso en línea:http://cds.cern.ch/record/1115632
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author CERN. Geneva
author_facet CERN. Geneva
author_sort CERN. Geneva
collection CERN
description <!--HTML-->Comets are kilometre-size aggregates of ice and dust, which remained from the formation of the solar system. It was not obvious to expect X-ray emission from such objects. Nevertheless, when comet Hyakutake (C/1996 B2) was observed with the ROSAT X-ray satellite during its close approach to Earth in March 1996, bright X-ray emission from this comet was discovered. This finding triggered a search in archival ROSAT data for comets, which might have accidentally crossed the field of view during observations of unrelated targets. To increase the surprise even more, X-ray emission was detected from four additional comets, which were optically 300 to 30 000 times fainter than Hyakutake. For one of them, comet Arai (C/1991 A2), X-ray emission was even found in data which were taken six weeks before the comet was optically discovered. These findings showed that comets represent a new class of celestial X-ray sources. The subsequent detection of X-ray emission from several other comets in dedicated observations confirmed this conclusion. The talk will summarise the highlights of the series of discoveries and provide an explanation for this unexpected phenomenon.<BR><BR><I>Organiser(s): Luigi Di Lella / EP Division</I><BR><BR><I>Note: Tea & coffee will be served at 16.00 hrs.</I>
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spelling cern-11156322022-11-02T22:20:14Zhttp://cds.cern.ch/record/1115632engCERN. GenevaX-rays from comets - a surprising discoveryX-rays from comets - a surprising discoveryCERN Colloquium<!--HTML-->Comets are kilometre-size aggregates of ice and dust, which remained from the formation of the solar system. It was not obvious to expect X-ray emission from such objects. Nevertheless, when comet Hyakutake (C/1996 B2) was observed with the ROSAT X-ray satellite during its close approach to Earth in March 1996, bright X-ray emission from this comet was discovered. This finding triggered a search in archival ROSAT data for comets, which might have accidentally crossed the field of view during observations of unrelated targets. To increase the surprise even more, X-ray emission was detected from four additional comets, which were optically 300 to 30 000 times fainter than Hyakutake. For one of them, comet Arai (C/1991 A2), X-ray emission was even found in data which were taken six weeks before the comet was optically discovered. These findings showed that comets represent a new class of celestial X-ray sources. The subsequent detection of X-ray emission from several other comets in dedicated observations confirmed this conclusion. The talk will summarise the highlights of the series of discoveries and provide an explanation for this unexpected phenomenon.<BR><BR><I>Organiser(s): Luigi Di Lella / EP Division</I><BR><BR><I>Note: Tea & coffee will be served at 16.00 hrs.</I>CERNoai:cds.cern.ch:11156322000
spellingShingle CERN Colloquium
CERN. Geneva
X-rays from comets - a surprising discovery
title X-rays from comets - a surprising discovery
title_full X-rays from comets - a surprising discovery
title_fullStr X-rays from comets - a surprising discovery
title_full_unstemmed X-rays from comets - a surprising discovery
title_short X-rays from comets - a surprising discovery
title_sort x-rays from comets - a surprising discovery
topic CERN Colloquium
url http://cds.cern.ch/record/1115632
work_keys_str_mv AT cerngeneva xraysfromcometsasurprisingdiscovery