A big group of stars is far away.
It is a bright spiral shape. It has long arms that spin. We can see it in the night sky. It helps us learn about space. Can you look for it?
A big group of stars is far away.
This group is a bright spiral shape. It has long arms that spin. It also has two extra arms. We see these with special tools.
There is a huge, heavy spot at the center. It pulls on gas nearby. This helps us find how far it is.
Two huge star deaths happened here too. This group is very large and bright. It is like our neighbor, the Andromeda group. It is a very special part of space.
Messier 106 is a big spiral galaxy.
It sits in the constellation Canes Venatici. Pierre Méchain found it in 1781. This galaxy is very large and bright. It is like the Andromeda Galaxy. It is 22 to 25 million light-years away.
At its center is a supermassive black hole. This is a huge, heavy spot. It pulls on a disk of gas. We can see this gas move with radio tools. M106 also has two strange arms. We see these arms with X-ray telescopes.
Scientists use a special tool called a water megamaser. This works like a laser but uses microwave light. It helps us measure how far away galaxies are. This helps us map the whole universe.
Two big star deaths happened here too. These are called supernovae. One happened in 1981. The other happened in 2014.
M106 might have a friend. A galaxy called NGC 4217 may be near it.
Messier 106 is a huge and bright spiral galaxy.
It sits in the constellation Canes Venatici. This galaxy is very similar to the Andromeda Galaxy. It is located about 22 to 25 million light-years away from Earth. Scientists call this type of galaxy an intermediate spiral galaxy. It is one of the largest and brightest galaxies nearby. This galaxy is very important for learning about space.
At the center of M106 is a supermassive black hole. This is a very heavy spot that pulls on things. A disk of molecular gas orbits around this center. We can see this gas move using radio-wavelength observations. This movement shows us the black hole is really there. The galaxy also has two special arms. These are called anomalous arms. We can only see them with an X-ray telescope.
M106 has a very cool feature called a water vapor megamaser.
A megamaser works like a laser. However, it uses microwave light instead of visible light. It happens on a very large galactic scale. This tool helps scientists see warm and dense gas. It also helps us study the disks around active galaxies. These masers helped us measure distances to galaxies for the first time.
Pierre Méchain discovered this galaxy in 1781.
M106 helps us build a cosmic distance ladder. This is a way to measure how far things are. The galaxy has Cepheid variables inside it. These are stars that help us find distances. They have metallicities similar to our own Milky Way. This helps us fix measurements for other galaxies too.
We can also see big star deaths in this galaxy. These events are called supernovae. One happened in 1981 and was called SN 1981K.
Another one called SN 2014bc was found in 2014. The 2014 event was found by the PS1 Science Consortium 3Pi survey. M106 might also have a companion galaxy. This possible friend is named NGC 4217. It is amazing to see how much is happening in one galaxy.
Messier 106 is a massive and bright intermediate spiral galaxy.
It is located in the constellation Canes Venatici. This galaxy is roughly similar in size and luminosity to the Andromeda Galaxy. It sits at a distance of about 22 to 25 million light-years from Earth. Astronomers classify M106 as a Type 2 Seyfert galaxy. This means it has a very active nucleus at its center. This active center is powered by a supermassive black hole. This black hole is a massive object that exerts a huge gravitational pull.
The center of M106 contains a very specific structure. A disk of molecular gas orbits within the inner light-year of the black hole. Scientists used radio-wavelength observations to watch this gas rotate. The way the gas moves proves that a supermassive black hole exists there. The galaxy also features a thin, slightly warped Keplerian disc. This disc is on a subparsec scale. It surrounds a central area with a very high mass. This structure is seen almost edge-on from our perspective.
M106 has different types of arms that stretch out from its center. Most people think of spiral galaxies as having two main arms. M106 does have two visible arms. However, it also possesses two "anomalous arms." These extra arms are not visible using regular optical light. We can only detect them by using an X-ray telescope.
The galaxy might also have a companion galaxy. This possible neighbor is named NGC 4217. These features show how complex a single galaxy can be.
One of the most unique features of M106 is its water vapor megamaser. A maser is similar to a laser. While a laser uses visible light, a megamaser operates on a galactic scale using microwave light. Specifically, M106 has a 22-GHz line of ortho-H2O. This provides evidence of dense and warm molecular gas. These water masers are very useful for scientists. They allow for the observation of nuclear accretion disks in active galaxies.
This process helps us see the environments around active galactic nuclei.
History shows that M106 has been studied for a long time. Pierre Méchain discovered the galaxy in 1781. Since then, it has helped scientists solve big mysteries about space. M106 played a vital role in calibrating the cosmic distance ladder. This ladder is a way to measure distances across the universe. Before M106, scientists struggled with Cepheid variables. These are stars used to measure distance. Cepheids in other galaxies often have different metallicities than those in the Milky Way.
This difference made them hard to use for accurate measurements.
M106 provided a solution to this measurement problem. It contains Cepheid variables with metallicities similar to our own Milky Way. By measuring these specific stars, astronomers could find a direct distance to the galaxy. This provided an independent anchor for the cosmic distance ladder. Once the distance to M106 was known, scientists could recalibrate other Cepheids. This is a fundamental step in improving how we quantify distances to other galaxies. It makes our entire map of the universe more accurate.
We can also observe massive stellar explosions in M106. These events are called supernovae. Two specific supernovae have been recorded in this galaxy. The first was SN 1981K, which was a Type II supernova. E. Hummel reported it, and Paul Wild verified it using archival photos from November 3, 1981. The second was SN 2014bc. This was also a Type II supernova with a magnitude of 14.8. The PS1 Science Consortium 3Pi survey discovered it on May 19, 2014.
These events help us understand the life cycles of stars.
Where will your curiosity go next?
🖼️ Images & Media (1)
More to explore
✨ What else?
Related topics you might enjoy
🔬 Go deeper
More advanced topics to explore
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.