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Kepler's Third Law of Planetary Motion01:18

Kepler's Third Law of Planetary Motion

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In the early 17th century, German astronomer and mathematician Johannes Kepler postulated three laws for the motion of planets in the solar system. In 1909, he formulated his first two laws based on the observations of his forebears, Nikolaus Copernicus and Tycho Brahe. However, in 1918, he published his third law of planetary motion, which gives a precise mathematical relationship between a planet's average distance from the Sun and the amount of time it takes to revolve around the Sun. It...
4.1K
Kepler's Second Law of Planetary Motion01:29

Kepler's Second Law of Planetary Motion

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In the early 17th century, German astronomer and mathematician Johannes Kepler postulated three laws for the motion of planets in the solar system. His first law states that all planets orbit the Sun in an elliptical orbit, with the Sun at one of the ellipse's foci. Therefore, the distance of a planet from the Sun varies throughout its revolution around the Sun.
While in an elliptical orbit, the total energy of the planet is conserved. Therefore, the planet slows down when it is at apogee and...
5.0K
Acceleration due to Gravity on Other Planets01:24

Acceleration due to Gravity on Other Planets

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The gravitational acceleration of an object near the Earth's surface is called the acceleration due to gravity. It can be measured by conducting simple experiments on Earth. However, such an experiment is impossible to conduct on the surface of other planets.
Astronomical observations are thus used to measure the acceleration due to gravity on other planets. This can be determined by observing the effect of a planet's gravity on objects close to it. The crucial factor that helps in this...
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Azimuths and Bearings01:19

Azimuths and Bearings

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Azimuths and bearings are essential concepts in surveying, providing methods to express the direction of a line relative to a meridian. Azimuths refer to the clockwise angle measured from the north end of a reference meridian to the given line, ranging from zero to 360 degrees. This method gives a comprehensive directional reference within a full 360-degree circle, making it a straightforward way to communicate direction in various fields, including navigation, cartography, and...
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Circular Orbits and Critical Velocity for Satellites01:16

Circular Orbits and Critical Velocity for Satellites

5.4K
The Moon orbits around the Earth. In turn, the Earth (and other planets) orbit the Sun. The space directly above our atmosphere is filled with artificial satellites in orbit. One can examine the circular orbit, the simplest kind of orbit, to understand the relationship between the speed and the period of planets and satellites with respect to their positions and the bodies that they orbit.
Nicolaus Copernicus (1473-1543) first suggested that the Earth and all other planets orbit the Sun in...
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Kepler's First Law of Planetary Motion01:10

Kepler's First Law of Planetary Motion

5.2K
In the early 17th century, German astronomer and mathematician Johannes Kepler postulated three laws for the motion of planets in the solar system. He formulated his first two laws based on the observations of his forebears, Nikolaus Copernicus and Tycho Brahe.
Polish astronomer Nikolaus Copernicus put forth a theory that stated a heliocentric model for the solar system. According to this heliocentric theory, all the planets, including Earth, orbit the Sun in circular orbits.
On the other hand,...
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Related Experiment Video

Updated: Dec 20, 2025

Scattering And Absorption of Light in Planetary Regoliths
11:34

Scattering And Absorption of Light in Planetary Regoliths

Published on: July 1, 2019

10.8K

ASTEROIDS OBSERVED FROM CS3: 2016 JULY - SEPTEMBER.

Robert D Stephens1

  • 1Center for Solar System Studies (CS3)/MoreData!, 11355 Mount Johnson Ct., Rancho Cucamonga, CA 91737 USA.

The Minor Planet Bulletin
|May 27, 2020
PubMed
Summary
This summary is machine-generated.

Twelve asteroids were observed using CCD photometry. These observations provide valuable data for understanding asteroid properties and solar system evolution.

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Area of Science:

  • Astronomy
  • Planetary Science
  • Solar System Studies

Background:

  • Asteroids are remnants from the early solar system.
  • Photometric observations are crucial for characterizing asteroid physical properties.

Purpose of the Study:

  • To conduct CCD photometric observations of twelve asteroids.
  • To gather data for asteroid characterization and solar system studies.

Main Methods:

  • Utilized CCD photometric observations.
  • Data collected at the Center for Solar System Studies.
  • Observations spanned from July to September 2016.

Main Results:

  • Acquired photometric data for twelve distinct asteroids.
  • Data provides a basis for further analysis of asteroid light curves and colors.

Conclusions:

  • The observational data contributes to the growing database of asteroid physical properties.
  • Further research can utilize this dataset to refine models of asteroid populations and solar system formation.