@Asbo Zaprudder I'm seing different values than those (like the ones in the linked chart) but I concede i am no expert.
en.wikipedia.org

Yes, different sources give different estimates. There doesn't appear to be a consensus. There is perhaps 50% uncertainty in the population percentages and the total number of stars in the Milky Way might be as low as 50 billion or as great as 400 billion. It's hard to tell because the solar system is embedded inside it. Being within a factor of two of the actual values would be an achievement. That between 75 and 80% are class M red dwarfs isn't in doubt - even given their lower luminosity.@Asbo Zaprudder I'm seing different values than those (like the ones in the linked chart) but I concede i am no expert.
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File:Stellar Classification Chart.png - Wikipedia
en.wikipedia.org
Oh I understand. Parsing the sources is also important. After all, you'll get different numbers if you consider all stars vs just main sequence stars.Yes, different sources give different estimates. There doesn't appear to be a consensus. There is perhaps 50% uncertainty in the population percentages and the total number of stars in the Milky Way might be as low as 50 billion or as great as 400 billion. It's hard to tell because the solar system is embedded inside it. Being within a factor of two of the actual values would be an achievement. That between 75 and 80% are class M red dwarfs isn't in doubt - even given their lower luminosity.
Neither of us are quoting the latest peer-reviewed scientific literature. I haven't had access to that for decades. Wikipedia is not a primary source. I was using http://www.atlasoftheuniverse.com/startype.html, specifically this graphic:Oh I understand. Parsing the sources is also important. After all, you'll get different numbers if you consider all stars vs just main sequence stars.
There are large uncertainties concerning the substellar region. In particular, the classical assumption of a single IMF covering the whole substellar and stellar mass range is being questioned, in favor of a two-component IMF to account for possible different formation modes for substellar objects—one IMF covering brown dwarfs and very-low-mass stars, and another ranging from the higher-mass brown dwarfs to the most massive stars. This leads to an overlap region approximately between 0.05–0.2 M☉ where both formation modes may account for bodies in this mass range.
At least Wikipedia does list their sources—and whenever possible, I do try to source those.Neither of us are quoting the latest peer-reviewed scientific literature. I haven't had access to that for decades. Wikipedia is not a primary source.
Assuming 100 billion stars, 8 percent would be 8 billion.90% of stars are on the main sequence so the numbers shouldn't be very different
There could be as many as many as 300 million potentially habitable planets in the Milky Way galaxy, according to research published in The Astronomical Journal. This is based on data from the Kepler space telescope and other research, which suggests that a significant percentage of Sun-like stars could host rocky planets within their habitable zones.
300 million is quite the number for our galaxy alone, but that doesn't mean they harbour life.
Additionally, we tend to look for carbon based life (not consider potentially life that could evolve that's NOT carbon based)... but even so, the possibility was proposed that there might be about 36 actively communicating civilisations in the galaxy.
In Star Trek, the Borg encountered 10026 species by the time VOY Dark Frontier happened... so that might be a TAD on the high end...
I think I read in some studies that it has been proposed that the potential number of intelligent civilisations in the Milky Way could be about 10,000.
The Milky Way alone may have billions to trillions of rogue planets, a range the upcoming Nancy Grace Roman Space Telescope is expected to refine.
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