Log in Sign up
Back to Discover
🚀

Rosette Nebula

space Maturity 11-13

A big cloud of gas is in space.

Rosette X-ray and Optical.jpg
Rosette X-ray and Optical.jpg
It looks like a rose. New stars grow inside it. These stars make the cloud glow. It is a pretty sight to see. Can you see the stars?
Rosette X-ray and Optical.jpg
Rosette X-ray and Optical.jpg

44 words

A big cloud of gas sits in space.

Rosette X-ray and Optical.jpg
Rosette X-ray and Optical.jpg
It looks like a rose. Some say it looks like a skull. Many new stars live inside the cloud. These young stars make the cloud glow. This happens because of light from the stars. There are about 2500 young stars there. It is a very large sight in the sky.
Rosette X-ray and Optical.jpg
Rosette X-ray and Optical.jpg

66 words

The Rosette Nebula is a giant cloud in space.

Rosette X-ray and Optical.jpg
Rosette X-ray and Optical.jpg
It is located in the Monoceros region. The nebula is about 130 light-years wide. It sits 5,000 light-years away from Earth. Some people say it looks like a rose. Others think it looks like a human skull.

Many young stars live inside this cloud. There are about 2,500 young stars there. These stars make the cloud glow. The stars give off radiation, which is a type of light. This light hits the atoms in the cloud. Then, the atoms give off their own light. This makes an emission nebula. This is the glowing cloud we see.

Two big stars are named HD 46223 and HD 46150. These are O-type stars. They help blow a big bubble in the cloud. There is also a hot glow between the stars. This is a super-hot plasma. Plasma is a very hot gas. It can be 1 to 10 million K hot. This heat comes from winds from the big stars.

Rosette X-ray and Optical.jpg
Rosette X-ray and Optical.jpg

Caption: Hundreds of young stars live inside the nebula.

183 words

The Rosette Nebula is a huge cloud in space. It is also called Caldwell 49. This cloud sits in the Monoceros region of our Milky Way Galaxy. It is an H II region, which is a type of glowing gas cloud. The nebula has a very interesting shape. Some people think it looks like a rose. Others say it looks like a human skull.

Rosette X-ray and Optical.jpg
Rosette X-ray and Optical.jpg

This nebula works by using light to glow. Inside the cloud, many young stars are forming. These stars give off radiation. This radiation hits the atoms in the nebula. Then, the atoms give off their own light. This creates what we call an emission nebula. Two massive O-type stars are named HD 46223 and HD 46150. These stars help blow a large bubble in the cloud.

Rosette X-ray and Optical.jpg
Rosette X-ray and Optical.jpg

Many people have studied this place over the years. John Flamsteed found the star cluster NGC 2244 in 1690. This cluster lives inside the nebula. John Herschel also discovered a part of the nebula called NGC 2239. The nebula is very far away. It is about 5,000 light-years from Earth. It is also very wide. The nebula is roughly 130 light-years across.

Rosette X-ray and Optical.jpg
Rosette X-ray and Optical.jpg

There are many specific facts about this star-forming area. The nebula has a mass of about 10,000 solar masses. There are about 2,500 young stars in this complex. Scientists found a hot glow between the stars. This is a super-hot plasma. It can be 1 to 10 million K. This heat comes from winds from the massive stars. The nebula also has several other names like NGC 2237 and NGC 2238.

Rosette X-ray and Optical.jpg
Rosette X-ray and Optical.jpg

You can think of the nebula as a giant star nursery. It is a place where new stars are born from gas. This is similar to how a garden grows flowers from soil. Even on Earth, we have special things for our stars. In 2019, Oklahoma made this nebula their official state astronomical object. Governor Kevin Stitt signed this law in April 2019. It is a very special place in our galaxy.

Rosette X-ray and Optical.jpg
Rosette X-ray and Optical.jpg

355 words

The Rosette Nebula is a massive H II region in our galaxy. An H II region is a large cloud of glowing gas. This nebula is located in the Monoceros region of the Milky Way. It sits near one end of a giant molecular cloud. Scientists also call this object Caldwell 49. It is a vital place for studying how stars are born. This nebula is a star-forming complex where new stars emerge from gas and dust.

Rosette X-ray and Optical.jpg
Rosette X-ray and Optical.jpg

The nebula works through a process of radiation and excitation. Inside the nebula, many young stars are constantly forming. These stars release intense radiation into the surrounding gas. This radiation hits the atoms within the nebula. This process is called excitation. When the atoms are excited, they emit their own radiation. This causes the cloud to glow with light. This specific type of glowing cloud is known as an emission nebula.

Rosette X-ray and Optical.jpg
Rosette X-ray and Optical.jpg

Several specific parts and objects make up this complex. The open cluster NGC 2244 is located inside the nebula. This cluster is also known as Caldwell 50. The stars in this cluster actually formed from the nebula's own matter. The nebula is divided into several cataloged parts. These include NGC 2237, NGC 2238, NGC 2239, and NGC 2246. There is also a smaller, less famous object called the Little Rosette Nebula. This is known as Sharpless 2-170.

Rosette X-ray and Optical.jpg
Rosette X-ray and Optical.jpg

History shows how astronomers have mapped this region over time. John Flamsteed discovered the star cluster NGC 2244 in 1690. Later, John Herschel discovered part of the nebula labeled NGC 2239. These discoveries helped us understand the relationship between stars and clouds. The nebula has also gained unique nicknames due to its shape. Some people call it the "Skull Nebula." However, this is different from another object called NGC 246.

Rosette X-ray and Optical.jpg
Rosette X-ray and Optical.jpg

The scale of the Rosette Nebula is truly enormous. It is located about 5,000 light-years away from Earth. The entire structure measures roughly 130 light-years in diameter. The total mass of the nebula is estimated at 10,000 solar masses. This means it weighs as much as 10,000 of our Sun. There are approximately 2,500 young stars in this star-forming complex. This massive amount of matter and energy shows how active the region is.

Rosette X-ray and Optical.jpg
Rosette X-ray and Optical.jpg

Recent studies have revealed surprising details about the nebula's environment. Massive O-type stars, such as HD 46223 and HD 46150, play a major role. These stars are powerful enough to blow an ionized bubble in the gas. The Chandra X-ray Observatory found a diffuse X-ray glow between the stars. This glow comes from a super-hot plasma. The temperature of this plasma ranges from 1 to 10 million K. This is much hotter than the 10,000 K plasmas found in other H II regions. This heat comes from shock-heated winds from the massive O-type stars.

Rosette X-ray and Optical.jpg
Rosette X-ray and Optical.jpg

The Rosette Nebula connects many different areas of science. It links the study of gas clouds to the birth of stars. It also connects X-ray astronomy to the study of massive stellar winds. Even on Earth, the nebula has special significance. On April 16, 2019, the Oklahoma Legislature passed HB1292. This law made the Rosette Nebula the official state astronomical object of Oklahoma. Governor Kevin Stitt signed the law on April 22, 2019. This shows how even distant space objects can connect to people on our planet.

Rosette X-ray and Optical.jpg
Rosette X-ray and Optical.jpg

577 words
🖼️ Images & Media (1)
File:Rosette X-ray and Optical.jpg
Rosette X-ray and Optical.jpg
Up Next
🚀
LBV 1806−20
Space
More to explore

🔬 Go deeper

More advanced topics to explore

🪜 Step back

Simpler topics to build understanding

What is Nepedia?

A free, ad-free encyclopedia for children. Every article is written at five reading levels, so the same page works for a five-year-old and a fifteen-year-old — use the level switcher above to see this one change. No account needed to read.