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Hubble captures brilliant star death in 'rotten egg' nebula

Date:
February 3, 2017
Source:
NASA/Goddard Space Flight Center
Summary:
The Calabash Nebula -- which has the technical name OH 231.8+04.2 -- is a spectacular example of the death of a low-mass star like the sun.
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The Calabash Nebula -- which has the technical name OH 231.8+04.2 -- is a spectacular example of the death of a low-mass star like the sun. This image taken by the NASA/ESA Hubble Space Telescope shows the star going through a rapid transformation from a red giant to a planetary nebula, during which it blows its outer layers of gas and dust out into the surrounding space.

The recently ejected material is spat out in opposite directions with immense speed -- the gas shown in yellow is moving close to one million kilometers per hour (621,371 miles per hour).

Astronomers rarely capture a star in this phase of its evolution because it occurs within the blink of an eye -- in astronomical terms. Over the next thousand years the nebula is expected to evolve into a fully-fledged planetary nebula.

The nebula is also known as the Rotten Egg Nebula because it contains a lot of sulphur, an element that, when combined with other elements, smells like a rotten egg -- but luckily, it resides over 5,000 light-years away in the constellation of Puppis.


Story Source:

Materials provided by NASA/Goddard Space Flight Center. Note: Content may be edited for style and length.


Cite This Page:

NASA/Goddard Space Flight Center. "Hubble captures brilliant star death in 'rotten egg' nebula." ScienceDaily. ScienceDaily, 3 February 2017. <www.sciencedaily.com/releases/2017/02/170203135054.htm>.
NASA/Goddard Space Flight Center. (2017, February 3). Hubble captures brilliant star death in 'rotten egg' nebula. ScienceDaily. Retrieved November 22, 2024 from www.sciencedaily.com/releases/2017/02/170203135054.htm
NASA/Goddard Space Flight Center. "Hubble captures brilliant star death in 'rotten egg' nebula." ScienceDaily. www.sciencedaily.com/releases/2017/02/170203135054.htm (accessed November 22, 2024).

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