Cookie consent

AstroBin saves small pieces of text information (cookies) on your device in order to deliver better content and for statistical purposes. You can disable the usage of cookies by changing the settings of your browser. By browsing AstroBin without changing the browser settings, you grant us permission to store that information on your device.

I agree
Getting plate-solving status, please wait...
NGC 7635 - The Bubble Nebula, 


            Hap Griffin

NGC 7635 - The Bubble Nebula

Technical card

Imaging telescope or lens:Planewave CDK 12,5'' 12.5 CDK

Imaging camera:QSI 583wsg

Mount:apt1200gto AP1200

Software:CCD Autopilot 5

Resolution: 1200x903

Dates:Aug. 8, 2010

Frames: 35x600"

Integration: 5.8 hours

Avg. Moon age: 27.66 days

Avg. Moon phase: 3.92% job: 1511836

Locations: ImagingInfinity Observatory, Bethune, SC, United States


Looking like a celestial Christmas tree ornament, this is the beautiful "Bubble Nebula", known officially as NGC7635. Is is formed by gas being compressed by a strong stellar wind from massive star BD+602522, forty times as massive as our sun and several hundred thousand times more luminous. As fast moving gas escapes the star, it compresses surrounding sparse gas into a shell. The shell, consisting of hydrogen, oxygen and sulfur, is ionized by the radiation from BD+602522 causing it to glow. The bubble is approximately 6 light-years in diameter.

BD+602522 is a "Wolf-Rayet" star, a star in the end stages of its life which emits fierce stellar winds (charged particles streaming from its surface) rapidly depleting its mass until it finally dies in a supernova. Wolf-Rayet stars (named for their discoverers) have surface temperatures between 30,000 and 60,000 degrees Kelvin and emit stellar winds with speeds exceeding 1500 kilometers per second. There are only about 300 Wolf-Rayet stars known in our galaxy.



Hap Griffin
License: None (All rights reserved)


NGC 7635 - The Bubble Nebula, 


            Hap Griffin