The Cosmic Perspective: Making Sense of the Universe (Chapter 4) Flashcards

(35 cards)

1
Q

The condition in which an object is falling without resistance

A

Free-fall

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2
Q

In the absence of a net force, an object moves with constant velocity

A

Newton’s First Law of Motion

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3
Q

Law states how a net force affects an object’s motion; force = mass X acceleration

A

Newton’s Second Law of Motion

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4
Q

For any force, there’s always an equal and opposite reaction of the force

A

Newton’s Third Law of Motion

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5
Q

The international unit of energy, equivalent to about 1/4000 of a Calorie

A

Joule

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6
Q

An encounter in which two (or more) objects pass near enough so that each can feel the effects of the other’s gravity and can therefore exchange energy

A

Gravitational Encounter

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7
Q

The most commonly used temperature scale in science is defined such that absolute zero is OK and water freezes at 273.15K

A

Kelvin

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8
Q

The temperature scale commonly used in daily activity internationally defined so that, on Earth’s surface, water freezes at 0 degrees Celsius and boils at 100 degrees Celsius

A

Celsius

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9
Q

The law expresses the force of gravity between two objects

A

Universal Law of Gravitation

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10
Q

Momentum attributable to rotation or revolution

A

Angular Momentum

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11
Q

The speed necessary for an object to escape the gravity of a large body (moon, planet, or star)

A

Escape Velocity

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12
Q

A law followed by any quantity that decreases with the square of the distance between two objects

A

Inverse Square Law

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13
Q

Orbits on which an object travels repeatedly around another object

A

Bound Orbits

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14
Q

The portion of any object’s total velocity that’s directed across our line of sight as it can only be measured by observing the object’s gradual motion across our sky

A

Tangential Velocity

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15
Q

The potential energy that can be released through chemical reactions

A

Chemical Potential Energy

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16
Q

The higher-than-average tides on Earth that occur at new and full moon, when the tidal forces from the Sun and Moon both act along the same line

17
Q

The amount of mass per unit volume of an object; it’s more commonly stated in units of grams/cubic centimeter in Astronomy

A

Density (Mass)

18
Q

The sum of an orbiting object’s kinetic and gravitational potential energies

A

Orbital Energy

19
Q

A measure of the average kinetic energy of particles in a substance

20
Q

The three basic laws that describe how objects respond to forces

A

Newton’s Laws of Motion

21
Q

The standard unit of force in the metric system

22
Q

The lower-than-average tides on Earth that occur at first- and third-quarter moon, when the tidal forces from the Sun and Moon oppose each other

23
Q

Energy carried by light

A

Radiative Energy

24
Q

A generalization of Kepler’s third law used to calculate the masses of orbiting objects from measurements of orbital period and distance

A

Newton’s version of Kepler’s third law

25
The precise mathematical shape of one type of unbound orbit (The other is a parabola) allowed under the force of gravity
Hyperbola
26
The coldest possible temperature, which is 0K
Absolute Zero
27
The proposed force that exists at very high energies when the strong, weak, and electromagnetic forces all act as one
GUT Force
28
Friction within an object that's caused by a tidal force
Tidal Friction
29
A force that occurs when the gravity pulling on one side of an object is larger than that on the other side, causing the object to stretch
Tidal Force
30
The rate at which an object's velocity changes; standard units are Mass/Speed^2
Acceleration
31
Energy stored for later conversion into kinetic energy; includes gravitational, electrical, and chemical potential energies
Potential Energy
32
The experimentally measured constant G that appears in the law of universal gravitation
Gravitational Constant
33
The collective kinetic energy, as measured by temperature, of the many individual particles moving within a substance
Thermal Energy
34
A weight of zero, as occurs during free-fall
Weightlessness
35
A satellite that orbits Earth in the same time it takes Earth to rotate (one sidereal day)
Geosynchronous Satellite