Tagged: Nebula - Adam Lundie - Eatons Hill Observatory

Tagged: Nebula

Prawn Nebula in Emission Line Color thumbnail
10-Aug-2018
IC 4628, sometimes known as The Prawn Nebula, is an emission nebula located around 6000 light-years away in the constellation Scorpius

Prawn Nebula in Natural Color thumbnail
10-Aug-2018
IC 4628, sometimes known as The Prawn Nebula, is an emission nebula located around 6000 light-years away in the constellation Scorpius

Cats Paw Nebula thumbnail
19-Jul-2018
Shaped like a cats paw, NGC 6334 is a stellar nursery and emission nebula 5,500 light years away in the constellation Scorpius. This image comprises of emission line data for Sulfur-II, Hydrogen-alpha and Oxygen-III, mapped to red, green, and blue respectively.

Ara Dragons NGC6188 thumbnail
04-Jul-2018
NGC 6188 is a large emission nebula of compressed molecular clouds 4,000 light years away in the constellation Ara. This image spans around 3 full moons and comprises of emission line data for Sulfur-II, Hydrogen-alpha and Oxygen-III, mapped to red, green, and blue respectively.

Shapley 1 Planetary Nebula thumbnail
04-Jun-2018
Shapley 1 is a planetary nebula in the southern sky with a magnitude 14 white dwarf at it's center. It is approximately 4900 light years away, and one third of a light year across.

Snake Nebula thumbnail
24-May-2018
The Snake Nebula (also known as Barnard 72) is a small but S-shaped dust lane that snakes out in front of the Milky Way star clouds.

Reflection Nebula NGC5367 thumbnail
25-Apr-2018
NGC5367 is a reflection nebula 2000 light years in the Centaurus constellation. The bright blue stars illuminate the otherwise dark molecular cloud complex.

Planetary Nebula NGC4361 thumbnail
18-Apr-2018
NGC4361 is a planetary nebula with spiral arms similar to a galaxy. The star at the center of the nebula is shedding its outer layers while contracting to form a white dwarf.

Gabriela Mistral Nebula thumbnail
13-Mar-2018
The Gabriela Mistral Nebula lies close to the Carina Nebula ~7500 light years distant in the far-southern sky. This image is a narrowband representation showing glowing ionised gasses, Hydrogen-alpha (orange), Sulfur-II (red), and Oxygen-III (blue).

Waves of Vela thumbnail
28-Jan-2018
The Vela Supernova Remnant is an expanding bubble of ionized gas 800 light years away, caused by a supernova explosion 12000 years ago. This image is a small section of the bubble, presented as a narrowband combination of light emitted by Hydrogen alpha, Sulfur II and Oxygen III.

Rosette Nebula thumbnail
21-Jan-2018
The Rosette Nebula is an emission nebula 3000 light years away. The central area of the nebula contains an open cluster of hot, blue stars which have cleared much of the center of its gas.

South of Orion - NGC1999 thumbnail
08-Jan-2018
NGC 1999 is a dusty blue reflection nebula, embedded in the hydrogen dust cloud of Orion. This narrow band enhanced image shows the light blue NGC 1999 at the center, with the edge of M42 (the Orion Nebula) at the far right. Also shown in the image is the waterfall nebula, the magenta shock wave between NGC 1999 and M42.

Robins Egg Nebula thumbnail
28-Nov-2017
NGC 1360 is known as the Robin's Egg Nebula, primarily due to its blue hue from strong oxygen-III emissions. It is a diffuse planetary nebula 1794 light years away. Presented is a narrowband image with H-alpha emissions mapped to red, and OIII emissions mapped to both green and blue (HOO palette).

Symbiotic Star System R Aquarii thumbnail
21-Sep-2017
R Aquarii is a symbiotic star system where a white dwarf is drawing material from its binary red giant companion. The extra material is then ejected into space in loops and jets.

Nebula Sh2-37 thumbnail
17-Aug-2017
Sh2-37 is a hydrogen emission nebula with two small blue reflection nebulae, embedded in a dusty background against the core of the Milky Way.

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