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M8

Lagoon Nebula

M8 EmissionNebula Sagittarius Visível Nível 3 Medium telescope (6-8") - Benefits from UHC/H-alpha filter
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Propriedades

Magnitude 4.6
Tamanho Angular 45.0′ × 30.0′
Distância 4100 ly
Emission Nebula [Distance: 4100 ly]

Posição e Identificadores

RA 18h 03m 37.0s
Dec -24° 23' 12.0"
Constelação Sagittarius
Catálogo M8

Visibilidade

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Imagem de Levantamento

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Sobre M8

Descrição

The Lagoon Nebula is one of the brightest and largest nebulae in the sky, located about 4,100 light-years away in the constellation Sagittarius. It is a giant interstellar cloud of gas and dust spanning about 110 by 50 light-years, with an associated young open cluster (NGC 6530) of about 50-100 hot young stars that illuminate the nebula. The prominent dark lane running through the center — which gives the nebula its 'lagoon' appearance — is a region of dense, obscuring dust.

Dicas de Observação

Located in a rich part of the Milky Way in Sagittarius, about 5 degrees north of the 'lid' of the Teapot asterism. Visible to the naked eye as a bright patch from dark sites. Binoculars reveal a large, bright nebula with the embedded star cluster NGC 6530. In a telescope at low power, the dark lagoon channel is clearly visible bisecting the nebula. Higher power reveals the Hourglass Nebula — a bright, compact region of turbulent gas near the center. Use a UHC or OIII filter to enhance nebular detail. Best observed from June through August when Sagittarius is at its highest.

História

Discovered by Giovanni Hodierna before 1654, making it one of the earliest nebulae observed telescopically. Independently discovered by John Flamsteed around 1680 and by Philippe Loys de Cheseaux in 1746. Charles Messier cataloged it in 1764. The Hourglass Nebula within M8 was first described by John Herschel, who also gave the Lagoon Nebula its common name.

Curiosidades

The Lagoon Nebula is one of only two star-forming nebulae visible to the naked eye from mid-northern latitudes (the other being M42). Hubble Space Telescope images of the Hourglass region reveal tornado-like structures — twisted funnels of gas shaped by the intense radiation from the hot young star Herschel 36. The nebula is estimated to be producing new stars at about 10 times the rate of the Orion Nebula.

Fotos da Comunidade (1)

Credit: National Science Foundation - Department of Energy Vera C. Rubin Observatory. License: CC BY 4.0. (Wikimedia Commons)

Credit: National Science Foundation - Department of Energy Vera C. Rubin Observatory. License: CC BY 4.0. (Wikimedia Commons)

Skybred Feb 28, 2026