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Comment Re:Practically alone... (Score 1) 307

Actually, it's only 17 million. A quick calculation gives me that the number of galaxies within 5 billion light-years is 170 million. Neglecting very small, dwarf galaxies, which are more numerous but have drastically fewer stars, I multiplied the stellar mass density by the comoving volume up to z=0.5.

Comment Re:I am dubious (Score 3, Interesting) 307

I can not answer about the deadliness of GRBs, but I think you will find those answers in Phil Plaits book "Death from the Skies!".

- How many civilizations might form on bodies with very thick atmospheres, far from their Suns? (Venus does not need a ozone layer to keep the UV out, and might be very habitable a few AU out.)

Yes, insulation is a good idea. But the planet will always radiate as a black body and loose energy, which has to be re-supplied by the suns radiation. The radiation drops with the square of the distance, so rather quickly. These considerations (make-up and size of planets) go into calculations for the habitable zone.

I can also imagine that a GRB comes with considerable photon pressure and might strip the entire atmosphere off a planet, or heat it to a point where it dissipates into space.

- How many planets might have very long rotation periods (years), so that the night hemisphere never is subjected to the daytime UV?

I think the rotation of planets around their own axis (spin) is not known outside the solar system. Generally, the spin is generated from formation of planets in the rotating protostellar disk, but interactions and changing orbits may modify the spin (Venus, Uranus).

- Are there rotation axis directions and orbital precession constants for planets that would keep GRB radiation mostly in one hemisphere, leaving the other to develop?

If you do not have the problem of heating and evaporation of the atmosphere I mentioned above, then yes, that is probably possible. For example if the GRB goes off from the direction of the spin axis ("below/above the solar system"). This may safe you from one GRB, but since GRBs come randomly from all directions it is not failsafe across many billion years.

- How many planets might have other special circumstances that protect their ozone (such as a lack of N2 in their atmosphere, or an ozone generating biology in their stratosphere, etc.)

Not sure. I think it is possible to come up with such scenarios as you stated, but it has to be shown that they are frequent occurrences to be relevant for changing the survival rate of complex life.

Comment Re:Let's do the math (Score 1) 307

While the Universe may be infinite, the Observable Universe is not infinite (limited by the speed of light).
The Universe within a radius of a certain number of light-years (and thus of age comparable to our location) is also finite. So considering the galaxies younger than 5 billion years, the number of those galaxies that can be observed (and can contain life that could communicate/meet with us) is finite.

A quick calculation gives me that the number of galaxies is 170 million. Neglecting very small, dwarf galaxies, which are more numerous but have drastically fewer stars, I multiplied the stellar mass density by the comoving volume up to z=0.5.

Comment Re:Huge Change (Score 2) 42

I was told, at a NSF meeting not many months ago, that CERN never makes its data openly available and never would and that US scientists should just plan on getting European collaborators if they want to work on it.

Now, if we just get ESA to start releasing the Rosetta data...

Most of the instruments (e.g. electronics) have a large US contribution. CERN operates the ring, but the instruments are "clients", which are international research teams. That was the vision of CERN after the second world war -- bring leading science to Europe, and make research in Europe attractive. Particle physics was chosen back then.

Comment Re:Go back in time 5 years (Score 1) 581

I think the way forward will be a lot of systemd forks that strip away functionality, and implement other functionality. That which will bring about the need for a common, standardized interface. And then, choice in init systems will be an option again (but timezoned, hostnamed, logind will be required).

Comment Re:Why do the browser teams write video code? (Score 1) 152

I don't get it. Why do the programmers working on browsers even write video support at all? No, I'm not saying browsers shouldn't support embedded video. But why does every browser have to reinvent that wheel? Isn't HTML, CSS and Javascript enough to have to support? I would think they would just link in libraries from a project which IS a video player like mplayer of xine or vlc or something. Then they should support whatever formats and framerates that player supports for free!

People tried that, 15-10 years ago. It did not work.
The reason it did not work is because it required every computer user to make sure their install is working, and the website could not fix setup problems. The user got the feeling that the website did not work and unusable. Sometimes this is justified, when you do not have install rights on the computer (e.g. labs). Websites started to offer plugin/viewer downloads, which caused a lot of malware problems.
Implementing it in the browser solves this problem. Implementation in HTML/CSS/JS on each website would not be enough, because the video data has to be streamed onto the graphic card for fast enough support.

Comment Complain to choosers, not creators (Score 2) 993

Complain to your distributions!
When someone writes open source software, it is always take it or leave it. Systemd was taken up, because it was the better solution for distros.
Why on earth would you complain about someone adding another choice? Complain about the people not writing alternative packages!

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