Dumbbell Nebula (M 27)

Name in the directory:M_27
Category:Nebula
Right Ascension:19h 59m 37.92s
Declination:+22° 43′ 23.16″
Total Exposure:6 часов 10 минут
Number of Frames:74
Link to FITS files:Download
  • 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.

PhotoDateFramesExposureLRGBHOSN
16 Jun 20227406:1000:2500:3000:2000:2002:0001:5000:45
24 Mar 20216505:2500:2500:3000:2000:2002:0001:50
18 Feb 20216505:2500:2500:3000:2000:2002:0001:50
20 Oct 20205804:5500:2500:3000:2000:2001:4001:40
26 May 20175000:2500:25
15 Aug 20156000:3000:30

Visibility chart of Dumbbell Nebula (M 27) during the day

The height diagram of Dumbbell Nebula (M 27) above the horizon during the current day for the observatory observation point in Orenburg (51.7, 55.2). The chart shows when the object is above the horizon and at what maximum height in degrees it rises. The data is relevant for the observation date: Saturday, 26 April 2025.
DateMoon PhaseExposureCCD TemperatureGainOffsetFilter
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