The Lagoon Nebula (catalogued as Messier 8 or M8, NGC 6523, Sharpless 25, RCW 146, and Gum 72) is a giant interstellar cloud in the constellation Sagittarius. It is classified as an emission nebula. It’s estimated to be between 4,000–6,000 light-years away.
The Lagoon Nebula (aka Messier 8) is an emission nebula estimated to be between 4,000-6,000 light-years away from the Earth. It’s a popular target for astrophotography. Here’s a view of M8 as seen by Hubble.
The Lagoon Nebula is a giant interstellar cloud in the constellation Sagittarius. It’s around 5,000 light-years from the Earth. As seen from Earth, it spans 90′ by 40′, which translates to an actual dimension of 110 by 50 light years.
The visible-light Hubble image of the Lagoon Nebula shows a dust-and-gas landscape that is being sculpted by ultraviolet radiation and stellar winds from a powerful young star. The star near the center of the image is known as Herschel 36. It’s about 200,000 times brighter than our Sun, 32 times more massive, and eight times hotter. Herschel 36 iis a baby star, only 1 million years old.
The star-filled image at right, taken by Hubble in near-infrared light, is a very different view of the nebula. Infrared light can penetrate clouds of gas and dust. The most obvious difference thes infrared and visible photos of this region is the abundance of stars that show up in the infrared field of view. Most of them are more distant, background stars located behind the nebula, but some are young stars within the Lagoon Nebula. The giant star Herschel 36 appears even brighter in infrared.
These Hubble Space Telescope images are views of the vast stellar nursery known as the Lagoon Nebula. One was taken in visible light (left) and the other in infrared (right).
The Lagoon Nebula, aka M8, is about 5,000 light years away in the constellation of Sagittarius. The center of the Lagoon Nebula is a maelstrom of star formation. The long funnel-shaped clouds on the lower left are roughly half a light-year long and have been formed by extreme stellar winds and intense energetic starlight. An extremely bright nearby star, Hershel 36, lights the area. Dust hides or reddens other hot young stars from our point of view. As energy from these stars flows into the cool dust and gas, the large temperature differences between adjoining regions can create generating shearing winds which may cause funnels to form.
This image shows the very rich region of sky centered around the Lagoon Nebula (Messier 8). The Trifid Nebula (Messier 20) is visible close to the top.
The Lagoon Nebula, also known as M8, lies about 5,000 light years distant toward the constellation of Sagittarius. Its center is a maelstrom of star formation. The two long funnel-shaped clouds near the center of the picture are each roughly half a light-year long. They were formed by extreme stellar winds and intense energetic starlight. An exceptionally bright nearby star, Herschel 36, dominates the area. Walls of dust hide and redden other hot young stars. This picture spans about 5 light years and combines several images taken by the Hubble Space Telescope.
Image Credit: Hubble Legacy Archive / NASA / ESA
Processing & License: Judy Schmidt
The Lagoon Nebula (aka Messier 8) is around 5000 light-years away in the constellation of Sagittarius (The Archer). It’s a cloud of gas and dust 100 light-years across where new stars are forming. The VLT Survey Telescope at ESO’s Paranal Observatory in Chile has captured a richly detailed new image of the Lagoon Nebula. The image is a tiny part of one of eleven public surveys of the sky now in progress using ESO telescopes. Together these are providing a vast legacy of publicly available data for the global astronomical community.