PSR J1856-3754 (Coronet Pulsar): Difference between revisions

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{{SystemInfobox|controller=Neutron Highway Initiative|government=Feudal|population=966.938|security=Low security|economy=Tourism|allegiance=Independent}}{{CelestialInfobox|startype=Neutron Star|age=574 million years|solarmasses=8,9023|solarradius=0|surfacetemp=985.067.520,00K|rotationalperiod=14,7D}}

{{SystemInfobox|controller=Neutron Highway Initiative|government=Feudal|population=966.938|security=Low security|economy=Tourism|allegiance=Independent|image=https://snipboard.io/96JEPQ.jpg}}{{CelestialInfobox|startype=Neutron Star|age=574 million years|solarmasses=8,9023|solarradius=0|surfacetemp=985.067.520,00K|rotationalperiod=14,7D}}

The 'Coronet' Pulsar is the colloquial term for the double neutron star system of PSR J1856-3754, the closest pulsar to Sol with a mere 521 light years. It lies in the Corona Austrinae molecular cloud and is associated with the so-called Coronet Cluster (CrA), a small cluster of young stars embedded in a small emission nebula (R CrA/NGC 6729) in that same region. The pulsar is also a member of the Magnificent Seven, a group of isolated neutron stars that are all relatively close to Sol and fall in line with the Gould Belt.

Revision as of 12:40, 1 June 2025 view source Fandom>Tranonica No edit summary ← Older edit		Latest revision as of 20:16, 16 May 2026 view source Fandom>Tranonica No edit summary
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	{{SystemInfobox\|controller=Neutron Highway Initiative\|government=Feudal\|population=966.938\|security=Low security\|economy=Tourism\|allegiance=Independent}}{{CelestialInfobox\|startype=Neutron Star\|age=574 million years\|solarmasses=8,9023\|solarradius=0\|surfacetemp=985.067.520,00K\|rotationalperiod=14,7D}}		{{SystemInfobox\|controller=Neutron Highway Initiative\|government=Feudal\|population=966.938\|security=Low security\|economy=Tourism\|allegiance=Independent\|image=https://snipboard.io/96JEPQ.jpg}}{{CelestialInfobox\|startype=Neutron Star\|age=574 million years\|solarmasses=8,9023\|solarradius=0\|surfacetemp=985.067.520,00K\|rotationalperiod=14,7D}}

	The 'Coronet' Pulsar is the colloquial term for the double neutron star system of PSR J1856-3754, the closest pulsar to Sol with a mere 521 light years. It lies in the Corona Austrinae molecular cloud and is associated with the so-called Coronet Cluster (CrA), a small cluster of young stars embedded in a small emission nebula (R CrA/NGC 6729) in that same region. The pulsar is also a member of the Magnificent Seven, a group of isolated neutron stars that are all relatively close to Sol and fall in line with the Gould Belt.		The 'Coronet' Pulsar is the colloquial term for the double neutron star system of PSR J1856-3754, the closest pulsar to Sol with a mere 521 light years. It lies in the Corona Austrinae molecular cloud and is associated with the so-called Coronet Cluster (CrA), a small cluster of young stars embedded in a small emission nebula (R CrA/NGC 6729) in that same region. The pulsar is also a member of the Magnificent Seven, a group of isolated neutron stars that are all relatively close to Sol and fall in line with the Gould Belt.

PSR J1856-3754 (Coronet Pulsar): Difference between revisions

Fandom>Tranonica