- 24,753
- 794
If anyone wants to work out a couple of recession speeds just to keep in practice.
The most distant OBJECT observed so far is the giant star at z = 8.3 that produced GRB 090423.
That was the big gammaray flash seen in April 2009.
Here is technical detail if anyone wants:
http://arxiv.org/abs/0902.2419
There is a great Perimeter video seminar talk just recently posted that discusses how they measure the redshift of these things and how they think the flashes are produced---by an unusual type of supernova of a rapidly spinning giant star where more happens than just the usual supernova mechanisms.
Or else by the abrupt merger of two compact objects like two neutron stars (abbreviated NS-NS)
or NS-BH. Eliot Quataert gives the talk.http://pirsa.org/09090028/
I'd say forget the technical paper, the Perimeter video is so good. A lot of the images are animated. The presenter, Eliot, is excellent. The latest understanding on how GRBs work.
Anyway try calculating the recession rate at the time the flash occurred, when the gamma started on its way to us. And also calculate the recession rate of the dead star remmant now today as the gamma arrives here. And the present distance.
What I get is that the expansion was 620 million years old when the flash occurred. And its age is about 13.7 billion years now. So the light has been traveling about 13 billion years.
See what you get. I used the old numbers: 0.27, 0.73, and 71 for matter fraction, cosmo constant, and present Hubble rate.
Some people might prefer the newer 0.25, 0.75, and 74. But it won't make a lot of difference, anything roughly around those values works OK.
What do you get for the two recession rates? the "now" and the "then" rate that the distance to the star was increasing.To repeat, this is the most distant object yet observed. The CMB is glow from hot gas, so not really an object. That hot gas is the most distant material observed--- redshift z = 1090---but the star that produced GRB 0904023 at z = 8.3 is the most distant condensed object.
Last edited: