Celestial hemisphere:  Northern  ·  Constellation: Cassiopeia (Cas)  ·  Contains:  Bubble Nebula  ·  HD220057  ·  HD240248  ·  HD240253  ·  LBN 544  ·  LBN 548  ·  LBN 549  ·  LDN 1231  ·  NGC 7635  ·  Sh2-162
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The Bubble Nebula, HR_Maurer
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The Bubble Nebula

Acquisition type: Electronically-Assisted Astronomy (EAA, e.g. based on a live video feed)
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The Bubble Nebula, HR_Maurer
Powered byPixInsight

The Bubble Nebula

Acquisition type: Electronically-Assisted Astronomy (EAA, e.g. based on a live video feed)

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Description

My version of the popular Bubble Nebula NGC 7635 in SHORGB.

Even though this nebula is shown very frequently, here some facts i gathered:
NGC 7635 is a HII region in constellation Cassiopeia in aproxinately 7000 LJ distance. A very young, hot 7.8 Mag O-star named BD +60° 2522 (~46 solar masses) is ejecting large amounts of stellar winds with velocities above 1800 km/s. These plasma winds form a heliosphere of about 7 LJ diameter, and finally crash into the surrounding molecular cloud. An approximately sperical shaped shock front established, where the kinetic energy of the lasma winds excite optical transitions we can observe in our telescopes, commonly in HII and [OIII]. For comparison, the heliosphere of our sun is approximately 2000 times smaller (roughly 200 AU in diameter, if a diameter can be defined).
The density of the cold surrounding medium is not uniform, so the shock front appears very off centered with respect to the origin of the winds (i didn't find any data about it's moving velocity with respect to the ISM). So, from our perspective, the O-star is located at a bubble radius of about 60%.
Moreover, the surrounding gas is excited by large amounts of ultraviolet light, while being pushed away, creating those beautiful finger-like structures with strong emission in Hydrogen, Nitrogen and Sulphur.

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