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Credit & Copyright: Adam Jensen
Explanation:
What excites the Heart Nebula?
First, the large emission nebula dubbed
IC 1805 looks, in whole, like a human heart.
Its shape perhaps fitting of the
Valentine's Day,
this heart glows brightly in red light
emitted by its most prominent element:
excited
hydrogen.
The red glow and the larger shape are all created by a
small group of stars near the
nebula's center.
In the heart of the
Heart
Nebula are young stars from the open star cluster
Melotte 15
that are eroding away several
picturesque dust pillars with their energetic light and winds.
The open cluster of stars contains a few
bright stars nearly 50 times the mass of our Sun,
many dim stars only a fraction of the mass of our Sun, and an
absent microquasar
that was expelled millions of years ago.
The Heart Nebula
is located about 7,500 light years away toward the
constellation
of the
mythological Queen of Aethiopia
(Cassiopeia).
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NASA Web Site Statements, Warnings, and Disclaimers
NASA Official: Jay Norris. Specific rights apply.
A service of: LHEA at NASA / GSFC
& Michigan Tech. U.
Based on Astronomy Picture
Of the Day
Publications with keywords: Heart Nebula - emission nebula - open cluster
Publications with words: Heart Nebula - emission nebula - open cluster
See also:
- Open Star Clusters M35 and NGC 2158
- APOD: 2025 February 25 Á M41: The Little Beehive Star Cluster
- APOD: 2025 February 18 Á Thors Helmet versus the Seagull
- APOD: 2025 February 11 Á The Spider and the Fly
- APOD: 2024 December 17 Á Near to the Heart Nebula
- The Elephant s Trunk in Cepheus
- APOD: 2024 October 29 Á NGC 602: Stars Versus Pillars from Webb