Chapter 3 Flashcards

(36 cards)

1
Q

Renaissance

A

A cultural movement spanning the 14th to 17th centuries that encompassed a flowering of education and art, much of which was based on principles established by the ancient greeks

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2
Q

Nicolaus Copernicus

A

developed a heliocentric model for the motions of the sun and planets in the solar system

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3
Q

Tycho Brahe

A

established the basis for a true understanding of planetary motion with naked-eye observations

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4
Q

Johannes Kepler

A

used Tycho’s meticulous observations of planet positions to develop his 3 laws of planetary motion

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5
Q

focus (foci)

A

either of two points interior to an ellipse that are used to define its shape. the sun is always at one focus of a planet’s elliptical orbit

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6
Q

first law of planetary motion

A

the principle by Johannes Kepler stating that planets move on elliptical orbits with the sun at one focus

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7
Q

semimajor axis

A

half of the long axis of an ellipse

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8
Q

semiminor axis

A

half of the short axis of an ellipse

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9
Q

eccentricity

A

a measure of the roundness of an ellipse, calculated as the ratio of the distance from the Earth’s center to its foci, divided by the length of the semimajor axis

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10
Q

perihelion

A

point closest to sun in a planets orbit

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11
Q

aphelion

A

point furthest from the sun in a planets orbit

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12
Q

second law of planetary motion

A

the Kepler principle stating that the line connecting a planet to the sun will sweep out equal areas of its orbit in equal times

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13
Q

conservation of angular momentum

A

the principle whereby a spinning or orbiting object increases its rotational speed as the radius (of either the spinning object or the object’s orbit) decreases, and vice versa

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14
Q

orbital period

A

the time an object takes to complete one revolution of an orbit

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15
Q

third law of planetary motion

A

the principle by Kepler stating that the square of a planet’s orbital period equals its average orbital radius cubed
P^2=R^3

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16
Q

Galileo Galilei

A

played an essential role in establishing the modern practices of sciences such as observation and experimentation. made discoveries with low-power telescopes that revolutionized astronomy.

17
Q

Galilean moons

A

the four largest moons of Jupiter: Io, Ganymede, Callisto, and Europa

18
Q

Sunspots

A

dark spots on the sun

19
Q

nebulosity

A

a word used by astronomers for clouds in space

20
Q

force

A

an interaction between two bodies that, if unbalanced, can change their state of motion

21
Q

mass

A

a property of matter that is related to its resistance to changes in motion or inertia. mass is measured in units of kilograms

22
Q

velocity

A

the change of a distance and the direction in which it is changing per unit of time

23
Q

speed

A

the change in distance per unit of time

24
Q

acceleration

A

the change of velocity per unit time

25
inertial law
principle advanced by isaac newton stating that objects in motion at constant velocity along a straight line continue that ay unless acted on by a net force
26
force law
principle advanced by isaac newton stating that the change in an object's acceleration due to an applied net force is in the same direction as the force and directly proportional to the object's mass
27
reaction law
the principle by isaac newton stating that for every applied force there is an equal and opposite force
28
momentum
the tendency of a moving object to continue in motion. only the application of a force can change an object's momentum
29
gravity
an attractive force between any two massive bodies that depends on the product of the bodies' masses and the inverse square of the distance between them
30
constant of nature
a term that does not change from one situation or time to another. the value of a constant of nature must be measured to be determined.
31
inverse square law
a relationship whereby a quantity (such as gravity) decreases in proportion to the square of a variable (such as distance) as the latter increases
32
weight
the force of an object that is produced by gravity
33
centripetal acceleration
acceleration involving a force that keeps an object moving on a curved path. the acceleration is directed toward the center of curvature of the path
34
centrifugal force
the illusion of outward force when an object is moving on a curved path
35
orbital velocity
the velocity required to keep a body in orbit around another body
36
escape velocity
the velocity required to escape the pull of gravity from a body