Tag Archives: M27

Dumbbell Nebula

63507ccf115a0f7cc008b082aeaa7de6.1824x0_q100_watermark_watermark_opacity-10_watermark_position-1_watermark_text-Copyright ray.gilman@cox.net

 

The Dumbbell Nebula (also known as Apple Core Nebula, Messier 27, M 27, or NGC 6853) is a planetary nebula in the constellationVulpecula, at a distance of about 1,360 light years.

This object was the first planetary nebula to be discovered; by Charles Messier in 1764. At its brightness of visual magnitude 7.5 and its diameter of about 8 arcminutes, it is easily visible in binoculars, and a popular observing target in amateur telescopes.

The Dumbbell Nebula appears to be shaped like an prolate spheroid and is viewed from our perspective along the plane of its equator. In 1992, Moreno-Corral et al. computed that its rate of expansion in the plane of the sky was no more than 2.3″ per century. From this, an upper limit to the age of 14,600 yr may be determined. In 1970, Bohuski, Smith, and Weedman found an expansion velocity of 31 km/s. Given its semi-minor axis radius of 1.01 ly, this implies that the kinematic age of the nebula is some 9,800 years.

Like many nearby planetary nebulae, the Dumbbell contains knots. Its central region is marked by a pattern of dark and bright cusped knots and their associated dark tails (see picture). The knots vary in appearance from symmetric objects with tails to rather irregular tail-less objects. Similarly to the Helix Nebula and the Eskimo Nebula, the heads of the knots have bright cusps which are local photoionizationfronts.

Imaging telescopes or lenses: Meade LX200 12″ GPS Pier mount
Imaging cameras: QSI 640 WSG-8
Mounts: Meade LX200 fork mount standard fork mount
Guiding telescopes or lenses: Borg 101ED/F6.4
Guiding cameras: SBIG STi-C
Focal reducers: Starizona SCT Corrector f/7.5
Software: Cyanogen Maxim DL5, Software Bisque TheSky
Filters: Astronomik Ha 12nm, Asronomik OIII , Astronomic SII 12nm
Accessories: Shoestring Astronomy FCUSB, Focuser JMI EVN-2
Resolution: 2048×2048
Dates: Oct. 1, 2014
Locations: Home Observatory
Frames: 33×300″
Integration: 2.8 hours
Avg. Moon age: 6.54 days
Avg. Moon phase: 41.10%
RA center: 299.901 degrees
DEC center: 22.708 degrees
Pixel scale: 0.722 arcsec/pixel
Orientation: -10.793 degrees
Field radius: 0.291 degrees

Autor: Ray G, 04.10.2014

M27 in Vulpecula

4d535e79e957762459bc5a200304923f.1824x0_q100_watermark_watermark_opacity-10_watermark_position-6_watermark_text-Copyright Marco Bocchini

The Dumbbell Nebula (also known as Apple Core NebulaMessier 27M 27, or NGC 6853) is a planetary nebula in the constellation Vulpecula, at a distance of about 1,360 light years.

This object was the first planetary nebula to be discovered; by Charles Messier in 1764. At its brightness of visual magnitude 7.5 and its diameter of about 8 arcminutes, it is easily visible in binoculars, and a popular observing target in amateur telescopes.

Imaging telescopes or lenses: Meade 10″ LX 200 ACF
Imaging cameras: Moravian G2-8300FW Moravian 8300
Mounts: Gemini g53F Gemini
Guiding telescopes or lenses: Meade 10″ LX 200 ACF
Guiding cameras: MagZero QHY5L-IIm
Software: PixInsight PinInsight 1.8, Maxim DL 5 MaximDL 5
Filters: Baader Planetarium Baader 1.25″ Ha SIII OII
Dates: Aug. 31, 2014
Frames: Baader Planetarium Baader 1.25″ Ha SIII OII: 40×1800″ -10C bin 1×1
Integration: 20.0 hours

Author: Marco Bocchini
AstroPhotography of the day by SPONLI 16 Sep 2014

M27: The Dumbbell Nebula

m27_snyder_2150
Image Credit & Copyright: Bill Snyder (Bill Snyder Photography)

 The first hint of what will become of our Sun was discovered inadvertently in 1764. At that time, Charles Messier was compiling a list of diffuse objects not to be confused with comets. The 27th object on Messier’s list, now known as M27 or the Dumbbell Nebula, is a planetary nebula, the type of nebula our Sun will produce when nuclear fusion stops in its core. M27 is one of the brightest planetary nebulae on the sky, and can be seen toward the constellation of the Fox (Vulpecula) with binoculars. It takes light about 1000 years to reach us from M27, shown above in colors emitted by hydrogen and oxygen. Understanding the physics and significance of M27 was well beyond 18th century science. Even today, many things remain mysterious about bipolar planetary nebula like M27, including the physical mechanism that expels a low-mass star’s gaseous outer-envelope, leaving an X-ray hot white dwarf.

APOD NASA 14-Sep-14

M27, the Dumbbell Nebula

16b125b6a311472bac0a1376f1687a67.1824x0_q100_watermark_watermark_opacity-16_watermark_position-4_watermark_text-Copyright Stefan Westphal

The Dumbbell Nebula (also known as Apple Core NebulaMessier 27M 27, or NGC 6853) is a planetary nebula in the constellation Vulpecula, at a distance of about 1,360 light years.

This object was the first planetary nebula to be discovered; by Charles Messier in 1764. At its brightness of visual magnitude 7.5 and its diameter of about 8 arcminutes, it is easily visible in binoculars, and a popular observing target in amateur telescopes.

Imaging telescopes or lenses: Orion Optics UK SPX 250
Imaging cameras: Canon 20Da
Mounts: Vixen New Atlux + Skysensor 2000
Guiding telescopes or lenses: Orion Optics UK SPX 250
Guiding cameras: M-Gen Guiding Kamera
Focal reducers: GPU Komakorrektor
Software: Adobe Photoshop CS2, DSS, Fitswork
Accessories: Lacerta MGEN2, Lacerta OAG
Dates: Sept. 6, 2013
Locations: Kreben
Frames: 44×360″ ISO800
Integration: 4.4 hours
Darks: ~20
Flats: ~11

Author: Stefan Westphal
AstroPhotography of the day by SPONLI 30 Aug 2014

Dumbbell Nebula

f929099d6116e7bf79f358e91fb756b7.1824x0_q100_watermark

The Dumbbell Nebula (also known as Apple Core NebulaMessier 27M 27, or NGC 6853) is a planetary nebula in theconstellation Vulpecula, at a distance of about 1,360 light years.

This object was the first planetary nebula to be discovered; by Charles Messier in 1764. At its brightness of visual magnitude 7.5 and its diameter of about 8 arcminutes, it is easily visible in binoculars, and a popular observing target in amateur telescopes.

Imaging telescopes or lenses: GSO RC8
Imaging cameras: Canon EOS 450D / Digital Rebel XSi / Kiss X2
Mounts: Sky-Watcher NEQ6
Guiding telescopes or lenses: Sky-Watcher 80/400
Guiding cameras: lacerta mgen2
Focal reducers: Teleskop-Service TS 2″ Flattener
Software: photoshop, PixInsight, Iris
Dates: June 23, 2012
Frames: 18×300″
Integration: 1.5 hours

Author:  Philippe Mingasson
AstroPhotography of the day by SPONLI 27 July 2014

Dumbbell Nebula in Vulpecula

831da340b90399b60be542a258410cac.1824x0_q100_watermark_watermark_opacity-10_watermark_position-6_watermark_text-Copyright FrancescoTallarico

The Dumbbell Nebula (also known as Apple Core NebulaMessier 27M 27, or NGC 6853) is a planetary nebula in the constellation Vulpecula, at a distance of about 1,360 light years.

This object was the first planetary nebula to be discovered; by Charles Messier in 1764. At its brightness of visual magnitude 7.5 and its diameter of about 8 arcminutes, it is easily visible in binoculars, and a popular observing target in amateur telescopes.

Imaging telescopes or lenses: Tecnosky Achromatic 152/900 f/5
Imaging cameras: Atik 383L+ mono
Mounts: Losmandy G11
Guiding telescopes or lenses: Tecnosky Achromatic 152/900 f/5
Guiding cameras: Starlight Xpress Lodestar
Software: DeepSkyStacker, Maxim DL, photoshop
Filters: OIII 12nm, Astronomik Ha
Accessories: OAG artigianale Turi Lo Vecchio
Frames:
Astronomik Ha: 33×900″ -15C bin 2×2
OIII 12nm: 31×900″ -15C bin 2×2
Integration: 16.0 hours
Darks: ~21
Flats: ~21
Bias: ~21
Mean FWHM: 3.00

Author: Francesco Tallarico
AstroPhotography of the day by SPONLI 07 May 2014

Dumbbell Nebula in the constellation Vulpecula

f82896774df826dec8fedf273c20ab58.1824x0_q100_watermark
The Dumbbell Nebula (also known as Apple Core NebulaMessier 27M 27, or NGC 6853) is a planetary nebula in the constellation Vulpecula, at a distance of about 1,360 light years. The Dumbbell Nebula appears to be shaped like an prolate spheroid and is viewed from our perspective along the plane of its equator.  The central star, a white dwarf, is estimated to have a radius which is 0.055 ± 0.02 R which gives it a size larger than any other known white dwarf. The central star mass was estimated in 1999 by Napiwotzki to be 0.56 ± 0.01 M.
This object was the first planetary nebula to be discovered.

Imaging telescopes or lenses: Meade SC 8″ LX-5
Imaging cameras: Nikon D5100
Mounts: Meade LX5
Guiding telescopes or lenses: Meade SC 8″ LX-5
Software: DeepSkyStacker, photoshop
Dates: July 29, 2012
Locations: Loowit Imaging Observatory
Frames: 30×50″
Integration: 0.4 hours

Author: Steve Rosenow

AstroPhotography of the day by SPONLI
10 April 2014