Objectives Flashcards
(40 cards)
What is the origin of the names of the days of the week?
7 Heavenly bodies which wander relative to fixed background stars. (Sun, Moon, Mars, Mercury, Jupiter, Venus, Saturn)
Parallax
An apparent change in position of an object due to an actual change in position of the observer.
Geocentric
An earth centered system
Heliocentric
A sun-centered system
Retrograde Motion
Planets seem to periodically reverse the direction of their wandering in the sky as the Earth passes by them in orbit with a greater velocity.
What is the diameter of the Earth?
Approximately 8,000 miles
Eratosthenes
Best early determination of Earth’s size
Ptolemy
Used epicycles to explain retrograde motion in geocentric system
Copernicus
Made 3 proposals which started Modern Astronomy
Tycho Brahe
Great Observer
Kepler
Formulated 3 famous laws. Worked w/Tycho
Galileo
1st to— •point telescope towards heavens •see mtns & craters on moon •detect 4 largest moons of Jupiter •phases of Venus •sunspots
3 Proposals made by Copernicus (and their implications)
- Stars are stationary. —>Earth rotates once daily.
- Sun is center of universe —>Earth revolves once yearly.
- Heavenly bodies move in perfect circles at constant speeds. —>epicycles only needed to account for variable speeds.
Distinguish between rotation and revolution
Rotation—spin around axis
Revolution—orbit around a body/focus
6 Proofs that Earth rotates
- Satellites in low Earth orbits change positions relative to Earth’s surface on each pass b/c satellite maintains original path while Earth rotates beneath it.
- Foucault pendulum
- Oblate spheroid shape of Earth.
- Falling objects fall to the East.
- Moon approaches at 600mph at moonrise; recedes at same rate at moonset.
- All weather formations are rotating. Effect of Coriolis forces.
Proofs of revolution
- Stellar Parallax. (The stars make little aloops.)
- Aberration of Starlight. Astronomers must tilt telescope to compensate for Earth’s rotational orbit.
- Certain stars approach us at one time, 6mo later receding.
Distinguish: Solar day & Sidereal day
Solar day: Measured w/respect to sun. 24hrs long.
Sidereal day: Measured w/respect to stars. (4min less)
Earth’s precessional angle
23.5° from vertical plane of orbit
Polaris is current N star
Seasons are result
Significance of Tropics of Cancer and Capricorn
Tropic of Cancer: Most N line on Earth’s surface where Sun rays hit vertically.
Tropic of Capricorn: Most S line where Sun directly overhead.
Arctic and Antarctic Circles
Arctic Circle: most S line in N hemisphere which can have sunlight for full 24hrs.
Antarctic Circle: most N line in S hemisphere that gets sunlight for full 24hrs.
Day, week, month, and year in astronomical terms.
Day: One rotation of Earth
Week: Possibly b/c 7 heavenly wanderers
Month: Moon’s revolution once around Earth
Year: One revolution of Earth around sun
Newton’s law of gravitation
F= (GMeMs)/(r^2)
4 Proofs that Earth is approx. spherical
- If flat—> objects moving away would only get smaller. B/c Earth has curvature—>objects slowly disappear over horizon.
- Shadow of Earth on moon is circular during an eclipse.
- Magellan’s voyage around world
- Pictures from space
Diameter of moon; distance to moon
2140; 240,000mi