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Spin Orbit Resonance

All articles tagged with #spin orbit resonance

Mercury’s Day Is Longer Than Its Year: 176 Earth-Day Sunrises
space2 months ago

Mercury’s Day Is Longer Than Its Year: 176 Earth-Day Sunrises

Mercury’s solar day (sunrise to sunrise) lasts 176 Earth days, because the planet spins once every 59 Earth days but orbits the Sun every 88 days, locking into a 3:2 spin-orbit resonance. As a result, a given spot on Mercury faces the Sun for two Mercury years before sunrise repeats, and the Sun can appear to rise, set, and rise again in a single day. This geometry—paired with a thin atmosphere—produces extreme day-night temperatures and explains why a “day” on Mercury is two years long, even though its year is just 88 days.

Seasons Beyond Earth: A Comparative Look at Planetary Variations
astronomy2 years ago

Seasons Beyond Earth: A Comparative Look at Planetary Variations

Earth's regular seasons are unique due to its slight tilt on its rotational axis, causing variations in sunlight throughout the year. This phenomenon, known as obliquity, can lead to drastic seasonal changes on other planets, with high obliquity resulting in extreme temperatures and reversed zonation. Spin-orbit resonances and the presence of moons can also influence a planet's obliquity and stability. Research on exoplanets, such as Kepler-186f, aims to understand the diversity of seasonal patterns across the universe.