Celestial hemisphere:  Northern  ·  Constellation: Cassiopeia (Cas)  ·  Contains:  Sh2-180
Getting plate-solving status, please wait...
SH2-180, Roland Schliessus
Powered byPixInsight
Getting plate-solving status, please wait...
SH2-180, Roland Schliessus
Powered byPixInsight

Equipment

Loading...

Acquisition details

Loading...

Description

SH2-180 is an emission nebula visible in the constellation Cassiopeia. It is located in the northwestern part of the constellation, approximately 2° ENE of the star κ Cassiopeiae; the most suitable period for its observation in the evening sky falls between the months of August and January and is considerably easier for observers located in the regions of the Earth's northern hemisphere, where it is circumpolar up to the warm temperate regions. Being at a distance of approximately 6100 parsecs (approximately 19900 light years), Sh2-180 is found on the Swan Arm, therefore beyond the large complexes linked to the OB associations visible in Cassiopeia, which almost all fall into the innermost arm of Perseus. It is believed that LS I +62 139, a blue main sequence star with spectral class O7.5V, is responsible for the ionization of its gases; estimates of its distance indicate for this star a value of 5150±1300 parsecs, which although smaller than the estimate of 6100 parsecs, is not very inconsistent with it given the considerable margin of uncertainty. Beyond these data, the nebula seems to have been little studied and its filamentary appearance, which resembles that of a supernova remnant, raises other questions.

====================== Source: Wikipedia ==========================

Comments