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Related Concept Videos

Kepler's First Law of Planetary Motion01:10

Kepler's First Law of Planetary Motion

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,...
Kepler's Second Law of Planetary Motion01:29

Kepler's Second Law of Planetary Motion

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...
Kepler's Third Law of Planetary Motion01:18

Kepler's Third Law of Planetary Motion

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...
Schwarzschild Radius and Event Horizon01:21

Schwarzschild Radius and Event Horizon

No object with a finite mass can travel faster than the speed of light in a vacuum. This fact has an interesting consequence in the domain of extremely high gravitational fields.
The minimum speed required to launch a projectile from the surface of an object to which it is gravitationally bound so that it eventually escapes the object’s gravitational field is called the escape velocity. The escape velocity is independent of the mass of the object. Merging the idea of escape velocity with the...
Detection of Black Holes01:10

Detection of Black Holes

Although black holes were theoretically postulated in the 1920s, they remained outside the domain of observational astronomy until the 1970s.
Their closest cousins are neutron stars, which are composed almost entirely of neutrons packed against each other, making them extremely dense. A neutron star has the same mass as the Sun but its diameter is only a few kilometers. Therefore, the escape velocity from their surface is close to the speed of light.
Not until the 1960s, when the first neutron...
Space-Time Curvature and the General Theory of Relativity01:17

Space-Time Curvature and the General Theory of Relativity

In 1905, Albert Einstein published his special theory of relativity. According to this theory, no matter in the universe can attain a speed greater than the speed of light in a vacuum, which thus serves as the speed limit of the universe.
This has been verified in many experiments. However, space and time are no longer absolute. Two observers moving relative to one another do not agree on the length of objects or the passage of time. The mechanics of objects based on Newton's laws of motion,...

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Related Experiment Video

Updated: Jul 24, 2026

Bringing the Visible Universe into Focus with Robo-AO
10:35

Bringing the Visible Universe into Focus with Robo-AO

Published on: February 12, 2013

Astronomy. Galactic encounters.

Rosemary Wyse1

  • 1Department of Physics and Astronomy, Johns Hopkins University, Baltimore, MD 21218, USA. wyse@skysrv.pha.jhu.edu

Science (New York, N.Y.)
|August 23, 2003
PubMed
Summary

The Milky Way galaxy has not experienced major collisions recently, unlike Andromeda. This galaxy formation study reviews satellite galaxy interactions and galactic evolution within the Local Group.

Area of Science:

  • Astronomy and astrophysics
  • Cosmic evolution and galaxy formation

Background:

  • The Local Group, including the Milky Way and Andromeda galaxies, provides a unique laboratory for studying galaxy formation and evolution.
  • Understanding galactic interactions, such as collisions with satellite galaxies, is key to deciphering cosmic history.

Purpose of the Study:

  • To review recent studies on collisions between the Milky Way and its satellite galaxies.
  • To compare the collision history of the Milky Way with that of the Andromeda galaxy.

Main Methods:

  • Review of observational data and theoretical models concerning galactic interactions within the Local Group.
  • Analysis of evidence for past collisions and accretion events in both the Milky Way and Andromeda.

Main Results:

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Last Updated: Jul 24, 2026

Bringing the Visible Universe into Focus with Robo-AO
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Scattering And Absorption of Light in Planetary Regoliths

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  • The Milky Way shows evidence of minor collisions, like with the Sagittarius dwarf galaxy.
  • The Milky Way appears to have avoided major collisions for the past 10 billion years, which is unusual for galaxy formation models.
  • Andromeda exhibits signs of significant recent accretion and/or disruption events, aligning better with expectations.

Conclusions:

  • The Milky Way's recent collision history deviates from typical galaxy formation models.
  • Andromeda's evolutionary path, marked by recent major events, offers a contrasting case study within the Local Group.