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ehkzu
Guest
Orpheus hit Earth, made the Moon outside the Roche limit, mainly from Earth's crust. Impact blows off excess water, makes dry continents possible. Moon stabilizes Earth's axial tilt, makes us possible. My question: is there any other plausible way for an Earthlike planet orbiting in its star's life zone to get a relatively big moon? <br /><br />I understand a capture is extremely unlikely--the planetoid would most likely just roll on by, its inertia overwhelming mutual gravitational attraction. Moreover, even if its relative velocity was so low as to make capture possible we'd still wind up with a water planet punctuated by just a few islands. Right? <br /><br />Second question: what would be a plausible range of sizes for a moon formed the way ours was? <br /><br />That is, how much bigger could it be before it caused such a tectonic ruckus on Earth as to make advanced life difficult?