Lunar volcanoes rock long-age timeframe

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Evolutionary timeframes date the moon at about 4.5 billion years, with the lunar volcanism that produced the large, prominent and nearly circular, dark “seas” (or maria, as they are called) starting soon after that. The volcanism is mooted to have ended about three billion years ago.

But researchers studying recent images of the far side of the moon, taken from the Japanese SELENE (Kaguya) lunar satellite, report dark “seas” of volcanic rock they say are “only” 2.5 billion years old, “much younger” than formerly presumed.1,2 That’s because there are fewer craters (blasted by meteors) on the smooth dark surfaces than expected—assuming the rate of cratering has been constant through time. Fewer craters means that the volcanic lava flows can’t be so old.

Given this volcanic activity lasted (supposedly) 500 million years later than previously thought, evolutionists now have the challenge of explaining how lunar volcanism was able to persist for so long. The moon is only about one-quarter the diameter of Earth, and only about one-eightieth of its mass, so it should have long ago cooled, and long been geologically dead.

Peeling back the uniformitarian assumptions, as our knowledge of space increases, mounting evidence points to the solar system (and the rest of the universe beyond) being much younger than the presumed evolutionary ages, consistent with the biblical time-frame of only around 6,000 years.3

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Source: creation.com

    

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