- O110 minutes (22 frames)
- R30 minutes (6 frames)
- H120 minutes (24 frames)
- S45 minutes (9 frames)
- L25 minutes (5 frames)
- B20 minutes (4 frames)
- G20 minutes (4 frames)
The Dumbbell Nebula (M27), also known as the Planetary Nebula, is one of the most famous and brightest objects in the night sky. It is located in the constellation Cygnus and was discovered by the French astronomer Charles Messier in 1764.
Name and Shape
The nebula gets its name from its shape, which resembles a dumbbell. It is a cloud of gas and dust that has expanded as a result of ejection of material from the core of a dying star. When viewed through a telescope, it appears as a bright ring or smoky cloud with a bright center.
Characteristics
- Diameter: about 2.5 light-years
- Distance from Earth: about 1,200 light-years
- Composition: The nebula contains various chemical elements, including hydrogen, helium, oxygen, and nitrogen — key building blocks for the formation of stars and planets.
Visibility
With a brightness of 7.5 magnitude, M27 is one of the brightest objects among planetary nebulae and is visible with telescopes even to amateur astronomers. It is especially easy to see in September.
Structure and study
- The nebula has the shape of an elongated spheroidal cloud, which is observed along the equator.
- In 1992, studies showed that its expansion rate is 2.3 arc seconds per century, which allows us to estimate its age at 14,600 years.
- In 1970, it was found that the expansion rate is 31 km/s, and according to this data, the age of the nebula can be estimated at 9,800 years.
- The central star of the nebula, which is a white dwarf, has a radius of about 0.055 solar radii and a mass of 0.56 solar masses.
Gas and dust knots
The nebula contains knots of gas and dust, which can be shaped like fingers pointing toward the central star, as well as clouds with and without tails. These knots vary in size from 17 to 56 billion kilometers, which is significantly greater than the distance from the Sun to Pluto.
Scientific Significance
Studying the Dumbbell Nebula allows astronomers to understand the processes that occur in dying stars and the evolution of nebulae. This research helps to expand our knowledge of the life cycle of stars and the formation of new star systems.
Popularity among Astronomers
The Dumbbell Nebula is an object of both professional research and a popular object for observation by amateur astronomers due to its brightness and unusual structure.
Visibility chart of Dumbbell Nebula (M 27) during the day
Date | Moon Phase | Exposure | CCD Temperature | Gain | Offset | Filter |
---|---|---|---|---|---|---|
- 2023ixf•
- 40 Eri•
- Abell 74•
- Artemis A868 SA•
- a Canis Minoris•
- C 2020 R4 ATLAS•
- C 2020 T2 Palomar•
- C 2021 S3 (PANSTARRS)•
- Haumea (2003 EL61)•
- HCG 68•
- HCG 92•
- IC 1318B•
- IC 1396•
- IC 1795•
- IC 1805•
- IC 1848•
- IC 1871•
- IC 3322A•
- IC 342•
- IC 4015•
- IC 405•
- IC 417•
- IC 434•
- IC 443•
- IC 4703•
- IC 5070•
- IC 5146•
- IC 63•
- M 1•
- M 101•
- M 103•
- M 109•
- M 13•
- M 15•
- M 27•
- M 3•
- M 33•
- M 42•
- M 45•
- M 5•
- M 51•
- M 57•
- M 63•
- M 64•
- M 74•
- M 76•
- M 81•
- M 82•
- M 86•
- M 87•
- M 94•
- M 97•
- NGC 147•
- NGC 1491•
- NGC 1499•
- NGC 1579•
- NGC 1961•
- NGC 2146•
- NGC 2239•
- NGC 2403•
- NGC 281•
- NGC 4236•
- NGC 4565•
- NGC 4631•
- NGC 507•
- NGC 508•
- NGC 5866•
- NGC 5907•
- NGC 6503•
- NGC 6823•
- NGC 6888•
- NGC 6946•
- NGC 6992•
- NGC 6995•
- NGC 7000•
- NGC 7023•
- NGC 7129•
- NGC 7217•
- NGC 7331•
- NGC 7380•
- NGC 7538•
- NGC 7635•
- NGC 7640•
- NGC 7822•
- NGC 891•
- NGC 896•
- NGC 925•
- PGC 54559•
- Sh2-155•
- Sh2-168•
- Sh2 103•
- Sh2 109•
- Sh2 132•
- T CrB•
- UGC 6930•
- V1405 Cas•
- Vesta A807 FA•