- How often does a star supernova? There are so many out there that it must be a fairly common occurence.
Sorry I don't have anything on your other questions (would simply be speculation on my part), but I can add a few points to this one. You're probably familiar with a lot of this, but I try to keep my posts well-rounded for others who might be reading.
It's important to remember that we don't just see stars in our galaxy, we also see stars in other galaxies. Naturally then, we can see supernovas in other galaxies. These occur quite frequently because there are a lot of galaxies out there. Here's a list of the ones we've seen:
http://www.cbat.eps.harvard.edu/lists/Supernovae.html (this answers your question in observational terms)
Now, obviously, we're not seeing all supernovae and we've only been observing for ~100 years (not including those which occurred in our own galaxy of which we have records for). Interestingly, we've actually discovered
supernova remnants*** in our galaxy which have matched up with historical observational records. E.g.,
SN 1006, which was widely observed on Earth back in 1006 CE, but the remnant was not discovered until 1965 when the region was observed using radio telescopes.
Now, to answer your question more directly, it's been estimated that one supernova occurs in the Milky Way every 50 years (
source). Obviously, we're seeing less than that. It's possible that our numbers are off, we're overdue, or we're just not seeing all of them due to interstellar dust. For reference, the Milky Way has 300 ± 100 billion stars (
source).
If we wanted to know how many are happening in the universe, we'd have to look at the number of stars in the universe, which is estimated to be somewhere between 3 to 100 * 10^22 (
source). Obviously, not all of those are going to go supernova, but if we assume a distribution of supernova-typical stars similar to the Milky Way, then we can do the following:
Milky Way rate: 1 every 50 years in a pool of 3 * 10^11
Universe rate: 1 every x years in a pool of 3 * 10^22
This gives us 1 * 10 ^ 11 supernovae every 50 years.
There are certainly a lot of factors I'm not considering, but that's an idea of how often they're happening.
*** As a personal aside, supernova remnants are one of my favourite things ever. The remnants weren't detected until the mid-1900s because they don't emit much in the visual wavelength and thus, weren't observed until we had things like radio and x-ray telescopes. However, the corresponding supernovae themselves were commonly observed by historical naked-eye observations. So, from those historical records and our current multi-wavelength observational data, we can determine how fast those supernovae are expanding, along with other properties.
It's one of those fantastic connections between historical scientific data and current scientific research.