Supriya Ghosh (Editor)

CG 4

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Right ascension
  
07 34 09.0

Distance
  
1,300 ly   (400 pc)

Declination
  
−46° 54′ 18″

Constellation
  
Puppis

CG 4

Dimensions
  
1.5 × 8 ly (0.46 × 2.45 pc)

Designations
  
BHR 21, DCld 259.4-12.7, FEST 2-30, Sandqvist 103

CG 4, commonly referred to as God's Hand, is a star-forming region located in the Puppis constellation, about 1,300 light-years (400 pc) from Earth. Its head is about 1.5 ly (0.46 pc) in diameter and its tail is about 8 ly (2.5 pc) long.

Contents

It is a cometary globule, one side of which has been blown outwards into a long tail, resembling a comet and hence named so. CG 4, and the nearby cometary globules, generally point away from the Vela Supernova Remnant, located at the center of the Gum Nebula.

Discovery

In 1976, photographs from the Schmidt Telescope—operated by the Australian Astronomical Observatory—showed several objects resembling comets, located in the Gum Nebula, an emission nebula of the constellation. Due to their particular shape, these objects came to be known as cometary globules. Each globule has a dense, dark, ruptured head and a very long tail, with the latter pointing away from the Vela Supernova Remnant. As a part of the ESO Cosmic Gems program, the European Southern Observatory released an image of CG 4 in January 2015 showing the head of the nebula.

Structure

The head of cometary globule CG 4 resembles a comet with a dusty cavernous mouth, as photographed by the European Southern Observatory's Very Large Telescope in 2015. Composed of relatively dense, dark matter, it is an opaque structure that is being illuminated by the glow of a nearby star. An obscure red glow limbing the globule is possibly caused by emission from ionized hydrogen. The mouth of the globule appears to be ready to consume the edge-on spiral galaxy ESO 257-19, located in the upper left corner of the image. In reality, the galaxy is over a hundred million light-years further away from the globule.

References

CG 4 Wikipedia