Star Formation: Rosette Nebula

Explore the Rosette’s layers
Full Story

Rosette Nebula Interactive

Dust and scattered stars surround a bright center
Crowded field of stars with dark gas clumps
Dark clouds surround a gas-filled area. Few stars visible
Scattered bright points which occasionally overlap Scattered bright points which occasionally overlap
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Stars forming within the Rosette Nebula heat layers of surrounding dust, giving them an infrared glow.

A cluster of young stars erodes the surrounding gas and dust, creating a central cavity within the Rosette Nebula.

The densest parts of the dust resist erosion, resulting in unique structures.

Ultraviolet light and stellar winds from young stars up to 50 times the mass of the Sun sculpt the nebula.

Infrared
Visible
Visible (Detail)
Ultraviolet

A Story Of Star Formation: Rosette Nebula

The most massive stars form the Rosette from the inside out.

Star formation is not truly a beginning, but is instead a phase in an ongoing recycling process in which gravity shapes new stars from the gas and dust expelled by old stars. Once formed, massive young stars shape the dusty nursery from which they form, blowing gas and dust out of some areas while compressing it in others. Forming stars are hidden inside thick cocoons of dust, emitting light in several wavelengths that pass through the dust clouds and can be detected by different telescopes.

Many of the Rosette Nebula’s most massive stars are concentrated in the center. At up to about 50 solar masses, their intense winds and high-energy light created the region’s central cavity. Visible light reveals the boundary where the gas and dust are carved by these stars. Hubble provides a look into a part of this boundary, showing where the stars have eroded all but the densest areas of dust and gas. Two types of dust — larger, sand-like carbon dust and smaller, soot-like hydrocarbon dust — are highlighted in the infrared wavelengths. The Rosette Nebula’s many layers will continue to change as more stars grow within.

Quick Facts: Rosette Nebula

Also known as: NGC 2237 and NGC 2244

Type of object: Star-forming nebula

Distance from Earth: 4,500 light-years

Size: 100 light-years across

Location in the sky: The constellation Monoceros (The Unicorn)

Did you know: The Wrench Trunk, a pillar with a claw-like head located toward the upper right of the central star cluster, has an unusual spiral shape that likely traces the magnetic field of the nebula.

Explore More About Star Formation

Find out more with these additional resources from NASA’s Universe of Learning

Credits: Rosette Nebula

Infrared image of the Rosette Nebula from WISE: NASA/JPL-Caltech/UCLA

Visible light image from the Dark Energy Camera (DECam) on the Víctor M. Blanco 4-meter Telescope at Cerro Tololo Inter-American Observatory: CTIO, NOIRLab, DOE, NSF, AURA

Visible light image of Rosette Nebula from the Hubble Space Telescope: NASA, ESA, STScI

Ultraviolet image of the Rosette Nebula from GALEX: NASA, STScI

Written, designed, developed, and produced by the Office of Public Outreach, Space Telescope Science Institute