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Cassiopeia A: Carbon Atmosphere Discovered On Neutron Star
Cassiopeia A

  • The neutron star at the center of Cas A is found to have an ultra-thin carbon atmosphere.

  • This atmosphere is uniformly distributed across the neutron star, explaining why there are no pulsations detected from this object.

  • The neutron star in Cas A was first detected over ten years ago in Chandra's "First Light" image.

This Chandra X-ray Observatory image shows the central region of the supernova remnant Cassiopeia A (Cas A, for short) the remains of a massive star that exploded in our galaxy. Evidence for a thin carbon atmosphere on a neutron star at the center of Cas A has been found. Besides resolving a ten-year-old mystery about the nature of this object, this result provides a vivid demonstration of the extreme nature of neutron stars. An artist's impression of the carbon-cloaked neutron star is also shown.

Discovered in Chandra's "First Light" image obtained in 1999, the point-like X-ray source at the center of Cas A was presumed to be a neutron star , the typical remnant of an exploded star, but it surprisingly did not show any evidence for X-ray or radio pulsations. By applying a model of a neutron star with a carbon atmosphere to this object, it was found that the region emitting X-rays would uniformly cover a typical neutron star. This would explain the lack of X-ray pulsations because this neutron star would be unlikely to display any changes in its intensity as it rotates. The result also provides evidence against the possibility that the collapsed star contains strange quark matter.

The properties of this carbon atmosphere are remarkable. It is only about four inches thick, has a density similar to diamond and a pressure more than ten times that found at the center of the Earth. As with the Earth's atmosphere, the extent of an atmosphere on a neutron star is proportional to the atmospheric temperature and inversely proportional to the surface gravity. The temperature is estimated to be almost two million degrees, much hotter than the Earth's atmosphere. However, the surface gravity on Cas A is 100 billion times stronger than on Earth, resulting in an incredibly thin atmosphere.

Fast Facts for Cassiopeia A:
Credit  X-ray: NASA/CXC/Southampton/W. Ho et al.; Illustration: NASA/CXC/M.Weiss
Release Date  November 4, 2009
Scale  Image is 4.5 arcmin across
Category  Supernovas & Supernova Remnants
Coordinates (J2000)  RA 23h 23m 26.7s | Dec +58° 49' 03.00"
Constellation  Cassiopeia
Observation Date  9 pointings in 2004: Feb 8, Apr 14, 18, 20, 22, 25, 28, May 01, 05
Observation Time  11 days, 14 hours
Obs. ID  4634-4639, 5196, 5319-5320
Instrument  ACIS
Also Known As Cas A
References W.Ho and C.Heinke, 2009, Nature (Nov 5 issue)
Color Code  Energy: Red (0.5-1.5 keV); Green (1.5-3.0 keV); Blue (4.0-6.0 keV)
X-ray
Distance Estimate  11,000 light years
Visitor Comments (8)

A couple of science fiction authors have speculated about the possibility of self-replicating structures life on neutron star surfaces, Robert Forward's novel "Dragon's Egg" is the most well-known example, and I think quite well-done.

Posted by Craig Heinke on Wednesday, 04.7.10 @ 10:12am


Dear Ed,
We give a reference to the Nature paper that was just published, and you
can also find the paper at:
http://lanl.arxiv.org/abs/0911.0672
-P. Edmonds, CXC

Posted by P. Edmonds on Tuesday, 11.10.09 @ 11:30am


Dear Marvin,
Thanks for your comment. The surface of a neutron star certainly wouldn't be the first place I would consider for the possibility of life, even very exotic life. The surface gravity and temperature, the magnetic fields and the atmosphere's density and pressure are all very high.
-P. Edmonds, CXC

Posted by P. Edmonds on Tuesday, 11.10.09 @ 11:28am


Congratulations,

You are on the right track. In fact there is a neutron star at the core of the Sun and probably of every other star.

The Sun and the cosmos are powered by neutron repulsion. I urge those at the Chandra Observatory to join the Yahoo Group, that Kirt Griffin established, to discuss the concept of neutron repulsion.

Please contact him or me for details.

With kind regards
Oliver K. Manuel

Posted by Oliver K Manuel on Saturday, 11.7.09 @ 06:37am


Thank you for info on Cassiopeia absolutely fascinating and very informative.

Posted by Gordon Musson on Friday, 11.6.09 @ 04:45am


Why is everything we discover strange? Answer we don't know squat. Keep exploring, learning, there is much out there.

Posted by Wayne C. Parker on Thursday, 11.5.09 @ 21:43pm


That is most interesting. I wonder what the significance of the carbon atmosphere is?
This may be too far out of a question, but we talk of the possibility of life on other planets, could there be the chance of there being a life as we do not know it living in stars or on or in their atmospheres. There was a SF short story I read long ago that speculated about this type of life.
Just a thought
Marvin L. S.

Posted by Marvin L S on Thursday, 11.5.09 @ 21:22pm


Sounds interesting, but explaining how was it established that this peculiar atmosphere is composed of carbon and that there is underneath an iron shell. And why does it prevent the pulsation - do not the shells rotate with the neutron star? At least a reference to a source or article where more details are available should be given with your reports.

Posted by Ed Bond on Thursday, 11.5.09 @ 18:01pm


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