Physical Science Course Outcome 4: Measurement, Motion, and Acceleration

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A collection of vocabulary flashcards based on the concepts covered in the Physical Science Course Outcome 4 lecture notes.

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17 Terms

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SI System

The International System of Units, a revised version of the metric system adopted by international agreement in 1960.

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Acceleration

In physics, it refers to the rate at which an object changes its velocity, including speeding up, slowing down, or changing direction.

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Newton’s 2nd Law of Motion

States that the force acting on an object is equal to the mass of that object multiplied by the acceleration of that object.

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Cubic Meter (m³)

The SI unit of volume, defined as the volume of a cube measuring 1 meter on each side.

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Kilogram (kg)

The base unit of mass in the SI system, originally defined as the mass of 1 liter of water at 4°C.

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Liter (L)

A non-SI unit of volume equal to the volume of a cube measuring 10 centimeters on each edge.

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Joule (J)

The SI unit of energy, equivalent to the amount of work done when a force of one newton displaces an object by one meter.

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Diurnal Motion

The apparent daily motion of celestial bodies across the sky due to the rotation of the Earth.

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Perihelion

The point in the orbit of a planet where it is closest to the sun.

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Aphelion

The point in the orbit of a planet where it is farthest from the sun.

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Summer Solstice

Occurs around June 21 when the Northern Hemisphere is tilted toward the sun, resulting in the longest day of the year.

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Winter Solstice

Occurs around December 21 when the Southern Hemisphere is tilted toward the sun, resulting in the shortest day of the year.

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Geocentric Theory

An ancient model of the universe that places Earth at the center.

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Heliocentric Theory

The astronomical model that places the Sun at the center of the universe with the Earth and other planets orbiting around it.

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Law of Ellipses

Kepler's first law, stating that the orbit of a planet around the sun is an ellipse with the sun at one of the two foci.

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Law of Equal Areas

Kepler's second law, which states that a line segment joining a planet and the sun sweeps out equal areas during equal intervals of time.

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Law of Harmonies

Kepler's third law, stating the square of a planet's orbital period is proportional to the cube of the semi-major axis of its orbit.