Celestial hemisphere:  Southern  ·  Constellation: Scorpius (Sco)  ·  Contains:  Bug Nebula  ·  NGC 6302  ·  PK349+01.1
Getting plate-solving status, please wait...
Bug Nebula,  NGC 6302, Frank Alvaro
Powered byPixInsight

Bug Nebula, NGC 6302

Getting plate-solving status, please wait...
Bug Nebula,  NGC 6302, Frank Alvaro
Powered byPixInsight

Bug Nebula, NGC 6302

Equipment

Loading...

Acquisition details

Loading...

Description

NGC 6302 (also known as the Bug Nebula, Butterfly Nebula, or Caldwell 69) is a bipolar planetary nebula 3800 light years away in the constellation Scorpius. The structure in the nebula is among the most complex ever seen in planetary nebulae. The spectrum of Butterfly Nebula shows that its central star is one of the hottest stars known, with a surface temperature in excess of 250,000 degrees Celsius, implying that the star from which it formed must have been very large. Hubble's Wide Field Camera 3 (WFC3) reveals a complex history of ejections from the star. The star first evolved into a red giant with a diameter of about 1,000 times that of our Sun. It then lost its extended outer layers. Some of this gas was cast off from its equator at a relatively slow speed, perhaps as low as 32,000 kph miles an hour, creating the torus. Other gas was ejected perpendicular to the ring at higher speeds, producing the elongated lobes or "wings" of the butterfly-shaped structure. Later, as the central star heated up, a much faster stellar wind (a stream of charged particles traveling at more than 3.2 million kph) plowed through the existing wing-shaped structure, further modifying its shape. (Wikipedia and hubblesite.org)

Comments