Chapter 2 Flashcards

(31 cards)

1
Q

Heliocentric

A

sun-centered model for the universe

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2
Q

Magnitude System

A

system devised by Hipparchus for describing brightness of stars

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3
Q

Prograde motion

A

eastward motion

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4
Q

Geocentric

A

Earth centered model for the universe

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5
Q

Epicycle

A

the circle path a planet travels around

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6
Q

Deferent

A

the larger circle which the epicycle moves at a constant speed around

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7
Q

Parallax

A

the shift in apparent position of an object when seen from two different locations

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8
Q

geocentric parallax

A

the shift in apparent position of a relatively nearby object

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9
Q

Heliocentric parallax

A

the shift in apparent position of a relatively nearby star when seen from two different points on the Earth’s orbit

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10
Q

Inferior Planets

A

those with orbits smaller than the Earth’s orbit (Mercury, Venus)

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11
Q

Superior Planets

A

those with orbits larger than the Earth’s orbit.

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12
Q

Opposition

A

occurs when the Earth lies between the Sun and the superior planet. The Sun and planet are 180 degrees apart

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13
Q

Conjunction

A

occurs when the Sun and the superior planet are 0 degrees apart as seen from the Earth

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14
Q

Quadrature

A

occurs when the Sun and the superior planet are 90 degrees apart as seen from the Earth, can be either eastern or western

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15
Q

Inferior conjunction

A

occurs when the inferior planet lies between the Earth and the Sun

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16
Q

Superior conjunction

A

occurs when the Sun lies between the Earth and the inferior planet

17
Q

elongation

A

the angle in which the planet is separated from the Sun on the celestial sphere

18
Q

Synodic period

A

time interval which can be found by measuring the time elapsed between either successive superior conjunctions or successive inferior conjunctions

19
Q

Sidereal period

A

the time it takes the planet to complete one full circuit of the sky relative to the fixed stars.

20
Q

Greatest elongation

A

the maximum angular separation between the planet and Sun as seen from the Earth

21
Q

Astronomical Unit

A

average distance from the Earth to the Sun

22
Q

Kepler’s first law

A

Planets travel on elliptical orbits with the Sun at one focus

23
Q

major axis

A

the longest distance across the ellipse

24
Q

minor axis

A

the shortest distance across the ellipse

25
eccentricity
the distance between the foci divided by the length of the major axis, if the foci coincide then the ellipse is a circle, e = 0
26
Kepler's second law
A line drawn from the Sun to a planet sweeps out equal areas in equal time intervals
27
perihelion
the point on a planets orbit closest to the Sun, (moves rapidly)
28
aphelion
the point farthest from the Sun, (least rapidly)
29
Kepler's third law
The squares of the sidereal orbital periods of the planets are proportional to the cubes of the semi-major axis of their orbits.
30
aberration of starlight
an effect that causes the apparent positions of stars on the celestial sphere to be deflected in the direction of the observer's motion.
31
parsec
the distance at which a star has a parallax of exactly 1 arcsecond