The moon formed about 4.4 billion years ago from a giant impact between Earth and a Mars-sized planet. The collision vaporized rock from both bodies, creating a massive gas cloud. Over time, this cloud cooled, and magma droplets clumped together to form the moon, which eventually emerged from the gas cloud and began orbiting Earth.
Earth and moon rocks are almost identical in geochemistry because they originated from the same material after the giant impact that formed the moon. The collision vaporized rock from both Earth and the impacting planet, creating a shared cloud of material that eventually condensed into the Earth and moon.
The moon is only about 1% the mass of Earth, meaning it lacks sufficient gravity to hold onto an atmosphere. Any gases released on the moon quickly escape into space due to its low gravity, leaving it airless and unable to support life.
Moonquakes are seismic activities on the moon caused by various factors, including temperature extremes and gravitational interactions with Earth. The moon's lack of atmosphere leads to extreme temperature shifts, causing the surface to expand and contract, which triggers quakes. Additionally, Earth's tides, influenced by the moon's gravity, create a feedback loop that affects the moon's surface.
The moon experiences extreme temperature variations, ranging from 250 degrees Fahrenheit in sunlight to -250 degrees Fahrenheit in shadow. This 500-degree difference occurs because the moon lacks an atmosphere to regulate heat, leading to rapid and drastic temperature changes.
Moon dust is razor-sharp because there is no wind or water on the moon to erode and smooth its particles. Without erosion, the dust remains jagged and can easily cut through materials, making it hazardous for astronauts and equipment.
Scientists have discovered ancient volcanoes on the moon, some billions of years old, with evidence of dried lava flows. These findings indicate that the moon was once geologically active, with volcanic eruptions shaping its surface.
The moon formed relatively quickly, taking about 10 to a few tens of years to condense from the gas cloud created by the giant impact. This rapid formation is a key aspect of the moon's origin story.
The giant impact that formed the moon also significantly altered Earth. It changed Earth's size, composition, and tilt, making it more habitable. Without this event, Earth might not have developed oceans, an atmosphere, or the conditions necessary for life.
Scientists have many unanswered questions about the moon, including the history of its impact events, the nature of its subsurface, the composition of its thin atmosphere, and why moonquakes are not observed on its far side. These mysteries highlight how much remains to be discovered about Earth's closest celestial neighbor.
The year’s best celestial event was, without a doubt, April’s solar eclipse. The moon went in front of the sun to cast a 115 mile wide shadow on Earth. A swathe of North America was showered in sudden darkness. In honor of the eclipse, the Radiolab team made a show about the star of the show: the moon.
We think we know the moon — we know that humanity visited it, that it’s a shiny white rotating rock in the sky. But what else really? In today’s episode, the team tells us about the moon’s formation, moon dust, moon-quakes, moon volcanoes, how the moon causes the tides on the Earth, and what the temperature up there is like. Turns out, we’ve barely scratched the surface.
For more, check out Rebecca Boyle’s book, ‘Our Moon: How the Earth’s Celestial Companion Transformed the Planet, Guided Evolution and Made Us Who We Are)’
Radiolab was created by Jad Abumrad and is edited by Soren Wheeler. Lulu Miller and Latif Nasser are our co-hosts. Dylan Keefe is our director of sound design. Our staff includes: Simon Adler, Jeremy Bloom, Becca Bressler, W. Harry Fortuna, David Gebel, Maria Paz Gutiérrez, Sindhu Gnanasambandan, Matt Kielty, Annie McEwen, Alex Neason, Valentina Powers, Sarah Qari, Sarah Sandbach, Arianne Wack, Pat Walters and Molly Webster. Our fact-checkers are Diane Kelly, Emily Krieger and Natalie Middleton. Production help from Tanya Chawla. Sound mixing by Joe Plourde.
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