These young stars become more benign, after about 250 million years, not into the billions of years as previously surmised. Thus, this now-widened time-window, for when calm, rocky planets like ours, in the Goldilocks Zone, might develop and retain warm oxygen rich atmospheres, and host water oceans. . . and thus see life arise. . . means many more systems might presently host. . . life. The chances are pretty darn good there is some life out there, somewhere -- but this slightly increases those already favorable odds. Here's that, from NASA | Goddard:
. . .Scientists have found that young stellar cousins of our Sun are calming down and dimming more quickly in their X-ray output than previously thought, according to a new study using NASA’s Chandra X-ray Observatory. A paper describing the results published Monday in The Astrophysical Journal.
Unlike in the new movie “Project Hail Mary,” this quieting of young stars is a benefit for the prospects for life on orbiting planets around these stars — not a threat.
Astronomers used Chandra and other telescopes to monitor how powerful radiation from young stars — often in the form of dangerous X-rays — can pummel planets surrounding them. They did not know, however, how long this high-energy barrage continued.
This latest study looked at eight clusters of stars between the ages of 45 million and 750 million years old. The researchers found that Sun-like stars in these clusters unleashed only about a quarter to a third of the X-rays they expected. . . .
The researchers found that stars with about the same mass as the Sun quieted down relatively rapidly — after a few hundred million years — while ones with less mass kept up their high levels of X-ray emission for longer. Combined with a decrease in the energy of the X-rays and the disappearance of energetic particles, the Sun-sized stars are apparently better suited to host planets with robust atmospheres and possibly blossoming life than previously thought. . . .
Of course, it may still be that "intelligent" life only lasts on these worlds for a few millenia, before destroying themselves with nukes, or destroying their host planets' environments -- to render them. . . barren, again.
That in turn may mean that we may never find our window is open at the same time, and within a distance that we might detect their presence. But the odds are high, that somewhere -- at some time out there. . . things like us have existed, or do now exist -- or will soon. . . exist.
Will we prove smart enough to avoid destroying ourselves long enough to meet them? Presently, I have my doubts. But onward, resolutely, just the same.
नमस्ते









No comments:
Post a Comment