Located approximately 7,500 light-years away in the Perseus Arm of our galaxy, the Heart Nebula (IC 1805) is a massive region of glowing gas and dark dust. Its distinctive shape, reminiscent of a human heart, makes it a favorite for astrophotographers, especially when paired with its neighbor, the Soul Nebula.
At the very center of the "heart" lies a small but incredibly powerful open cluster of stars known as Melotte 15. These stars are the "engine" that gives the nebula its life.
Massive Residents: This cluster contains a few young, hot stars that are nearly 50 times the mass of our Sun.
Sculpting the Gas: The intense radiation and stellar winds from these stars act like cosmic chisels, eroding the surrounding clouds into jagged pillars and deep ridges.
The Microquasar Mystery: Astronomers believe Melotte 15 once hosted a microquasar (a small black hole or neutron star), but it was violently expelled from the cluster millions of years ago.
The Heart Nebula is a classic emission nebula. It glows a deep, vivid red because it is primarily composed of ionized hydrogen gas.
When the ultraviolet light from the stars in Melotte 15 hits the hydrogen atoms, it strips away their electrons.
As those electrons recombine with the atoms, they release energy in the form of red light (specifically the Hydrogen-alpha wavelength).
In "Hubble Palette" images, you will also see blues and oranges, which represent ionized oxygen and sulfur.
If you look at the "bottom right" tip of the heart, you'll find a particularly bright and dense knot of gas. This region is separately cataloged as IC 1795, but it is more commonly known as the Fish Head Nebula.
It was actually the first part of the complex to be discovered (as NGC 896) because it is much brighter than the rest of the sprawling heart structure.
The Heart Nebula is far larger than it appears in small telescope views.
Physical Size: It spans roughly 330 light-years across.
Apparent Size: In the night sky, it covers an area about four times the size of the full moon.