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Insights on Mercury: The Elusive Planet
Sep 25, 2024
Lecture Notes: Mercury
Overview
Mercury is the closest planet to the Sun.
Known for extreme temperature variations.
One of the seven naked-eye solar system objects.
Associated with the Roman messenger god, known for its speed.
Historical Observations
Mercury's motion observed by Giovanni Zupi in 1639.
Exhibits phases like the Moon, proving it orbits the Sun.
Supports heliocentrism.
Orbit and Rotation
Average distance from the Sun: 58 million km (1/3 of Earth's distance from the Sun).
Rapid orbital movement due to proximity to the Sun.
Completes an orbit in 88 Earth days.
Phases observed due to relative positions to Earth and Sun.
Elliptical orbit: closest at 46 million km and farthest at 70 million km.
Spin-Orbit Resonance
Unique 2:3 spin-orbit resonance.
One day on Mercury lasts 59 Earth days.
Tidal forces once slowed Mercury's rotation.
At perihelion, one side faces the Sun and 1.5 spins later, the opposite side faces the Sun.
This results in a peculiar day length of 176 Earth days.
Surface and Atmosphere
Small size: 4900 km in diameter (1/3 of Earth's width).
Bright due to proximity to Sun but hard to observe due to horizon position.
Mapped by Mariner 10 and MESSENGER probes.
Surface is rocky with extensive cratering.
Notable features include Caloris Basin and "rupes" or compression folds.
Magnetic Field and Core
Has a magnetic field despite slow rotation.
Dense with a large iron core, possibly from a past grazing impact.
Core may reach Âľ of the way to the surface.
Atmospheric Conditions
Minimal atmosphere with traces due to solar wind and impacts.
Long comet-like tail made of elements like sodium and magnesium.
Impact Events
Craters formed by high-velocity impacts due to Mercury's fast orbit.
Ice on Mercury
Water ice exists in deep craters at the poles.
Ice located in "cold traps" where sunlight never reaches.
Likely sourced from comet/asteroid impacts.
Interesting Facts
Ice on a planet with extremely high surface temperatures.
Mercury's environmental conditions demonstrate nature's complexity.
Acknowledgements
Lecture by Phil Plait with contributions from Blake de Pastino and Dr. Michelle Thaller.
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