shadron
26th August 2009, 02:37 PM
In my pursuit of catastrophe stories, I just viewed the recently released the video: The Universe - Death Stars. It was done by the History channel and seems to have an unusual amount of "gloom-doom -repent now and buy our insurance" sort of urgency, not to speak of the breathless errors the narrative/narrator interject. "Igniting the ozone layer", with the repeated imagery of an recurve archer with a flaming arrow either hitting or missing an NAA-approved Olympic competition 70 meter target face at the range of perhaps 20 meters, forsooth. Far out.
The first of several problems discussed was that of WR-104, a binary star pair about 8000 LY form here. Both of the stars are at about 20x sun mass, and so have great potential for going nova soon. One of the two is a Wolf-Rayet (W-R) star, which continuously throws off an exterme amount of its mass as solar wind. The speculation is that the W-R star is capable of causing a gamma ray burst (GRB). WR-104 was described in a set of papers by Peter Tuthill in 2009. Of particular interest is that the two stars interact to focus the WR stars emissions into a spiral that moves outwards. The spiral seems to be face onto us (Tuthill estimates that we are no more than 16 degrees from the axis) which potentially brings us into the GRB focus if/when the WR goes nova. At the range of 8000ly the results may be pretty bad for us. Phil wrote this up on his Bad Astronomy blog; another recent paper brings the exact angle that we are viewing the spiral into question: http://www.universetoday.com/2009/01/07/wr-104-wont-kill-us-after-all/
For those who have astronomy backgrounds, I'd like to ask the following questions:
1. Is a W-R star particularly prone, theoretically, to cause a GRB? I see a lot of equivocation about this in the papers I've read.
2. Is the assumption that the W-R star's spin equator (which defines the axis of the GRB, as I understand it) equates to the spiral's "equator", which I presume matches the ecliptic of the binary star system, a good assumption? Out of suriosity, what about the other star?
3. I understand that trying to measure a presumed major and minor axis of the spiral, in order to see if we are face onto it or not is going to be frought with large error estimates, but is the difference between Tuthill's "0-16 degrees" vs the later "30-40, perhaps 45 degrees" a reasonable observational difference?
4. Are there other considerations which may make the spiral appear space-front when it actually isn't? I understand that the spiral is an observational phenomenon, that the actual particles making it up are travelling outwards radially; could they be excited in an unusual manner or some such so that the spiral itself is not indicative of the ecliptic/axis of the two stars?
The first of several problems discussed was that of WR-104, a binary star pair about 8000 LY form here. Both of the stars are at about 20x sun mass, and so have great potential for going nova soon. One of the two is a Wolf-Rayet (W-R) star, which continuously throws off an exterme amount of its mass as solar wind. The speculation is that the W-R star is capable of causing a gamma ray burst (GRB). WR-104 was described in a set of papers by Peter Tuthill in 2009. Of particular interest is that the two stars interact to focus the WR stars emissions into a spiral that moves outwards. The spiral seems to be face onto us (Tuthill estimates that we are no more than 16 degrees from the axis) which potentially brings us into the GRB focus if/when the WR goes nova. At the range of 8000ly the results may be pretty bad for us. Phil wrote this up on his Bad Astronomy blog; another recent paper brings the exact angle that we are viewing the spiral into question: http://www.universetoday.com/2009/01/07/wr-104-wont-kill-us-after-all/
For those who have astronomy backgrounds, I'd like to ask the following questions:
1. Is a W-R star particularly prone, theoretically, to cause a GRB? I see a lot of equivocation about this in the papers I've read.
2. Is the assumption that the W-R star's spin equator (which defines the axis of the GRB, as I understand it) equates to the spiral's "equator", which I presume matches the ecliptic of the binary star system, a good assumption? Out of suriosity, what about the other star?
3. I understand that trying to measure a presumed major and minor axis of the spiral, in order to see if we are face onto it or not is going to be frought with large error estimates, but is the difference between Tuthill's "0-16 degrees" vs the later "30-40, perhaps 45 degrees" a reasonable observational difference?
4. Are there other considerations which may make the spiral appear space-front when it actually isn't? I understand that the spiral is an observational phenomenon, that the actual particles making it up are travelling outwards radially; could they be excited in an unusual manner or some such so that the spiral itself is not indicative of the ecliptic/axis of the two stars?