Celestial hemisphere:  Southern  ·  Constellation: Dorado (Dor)  ·  Contains:  HD269989  ·  HD270016  ·  HD270032  ·  HD270055  ·  HD270076  ·  HD270119  ·  HD38941  ·  HD38942  ·  HD39282
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Henize 70 / N70, John Dziuba
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Henize 70 / N70

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Henize 70 / N70, John Dziuba
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Henize 70 / N70

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Description

Henize 70 is an emission nebula and superbubble located in the Large Magellanic cloud, a satellite galaxy to our Milky Way.  It is located roughly 160,000 light years away and has a diameter of roughly 300 light years.

Superbubbles are large expanding areas of interstellar gas, being blown outwards by winds from hot, massive stars and supernova explosions.  Their interiors are less dense than the surrounding medium with the intense winds, passage and gravity of newly born stars stripping the superbubbles of most internal dust and gas. 

At the center of Henize 70 is a small group of extremely hot and massive stars. Some of these stars are rapidly losing mass and have stellar winds blowing from their surfaces with velocities that approach 4000 kilometers per second. 

Because the lifetimes of massive stars are measured in only tens of millions of years, after one supernova has swept clear a bubble around itself, there isn’t enough time for the interstellar medium to back-fill the cavity before other stars explode in the same region. Each subsequent supernova will rejuvenate the cavity left by the previous ones. 

Our own Solar System lies near the center of an old superbubble, known as the Local Bubble, whose boundaries can be traced by a sudden rise in dust extinction of exterior stars at distances greater than a few hundred light years.

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    Henize 70 / N70, John Dziuba
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    Henize 70 / N70, John Dziuba
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Henize 70 / N70, John Dziuba