Search research articles

ABOUT JoVE

Overview Leadership Blog JoVE Help Center

AUTHORS

Publishing Process Editorial Board Scope & Policies Peer Review FAQ Submit

LIBRARIANS

Testimonials Subscriptions Access Resources Library Advisory Board FAQ

RESEARCH

JoVE Journal Methods Collections JoVE Encyclopedia of Experiments Archive

EDUCATION

JoVE Core JoVE Business JoVE Science Education JoVE Lab Manual Faculty Resource Center Faculty Site

Terms & Conditions of Use

Related Concept Videos

Kepler's First Law of Planetary Motion

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 Motion

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 Motion

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...

Acceleration due to Gravity on Other Planets

Acceleration due to Gravity on Other Planets

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...

Reduced Mass Coordinates: Isolated Two-body Problem

Reduced Mass Coordinates: Isolated Two-body Problem

In classical mechanics, the two-body problem is one of the fundamental problems describing the motion of two interacting bodies under gravity or any other central force. When considering the motion of two bodies, one of the most important concepts is the reduced mass coordinates, a quantity that allows the two-body problem to be solved like a single-body problem. In these circumstances, it is assumed that a single body with reduced mass revolves around another body fixed in a position with an...

One-Degree-of-Freedom System

One-Degree-of-Freedom System

In mechanical engineering, one-degree-of-freedom systems form the basis of a wide range of electrical and mechanical components. Using these models, engineers can predict the behavior of various parts in a larger system, which gives them insight into how different forces interact with each other.
A one-degree-of-freedom system is defined by an independent variable that determines its state and behavior. One example of a one-degree-of-freedom system is a simple harmonic oscillator, such as a...

You might also read

Related Articles

Articles linked to this work by shared authors, journal, and citation graph.

Sort by

Same author

Introduction to the Special Collection of Papers from EANA 2013: The 13th European Workshop on Astrobiology ("Through Cosmic Dust to DNA"): 22-25 July 2013, Szczecin, Poland.

Origins of life and evolution of the biosphere : the journal of the International Society for the Study of the Origin of Life·2014

Same author

Cosmic rays: a review for astrobiologists.

Astrobiology·2009

See all related articles

Search research articles

Related Experiment Video

Updated: May 21, 2026

Simulation of the Planetary Interior Differentiation Processes in the Laboratory

Simulation of the Planetary Interior Differentiation Processes in the Laboratory

Published on: November 15, 2013

Migration-induced architectures of planetary systems.

Ewa Szuszkiewicz¹, Edyta Podlewska-Gaca

¹CASA* and Institute of Physics, University of Szczecin, Szczecin, Poland. szusz@fermi.fiz.univ.szczecin.pl

Origins of Life and Evolution of the Biosphere : the Journal of the International Society for the Study of the Origin of Life

|June 12, 2012

Summary

Planetary systems with resonant configurations offer insights into planet formation. Studying these systems helps understand orbital migration and its role in shaping stable planetary architectures, crucial for habitability.

More Related Videos

Surface Mapping of Earth-like Exoplanets using Single Point Light Curves

Surface Mapping of Earth-like Exoplanets using Single Point Light Curves

Published on: May 10, 2020

Laboratory Drop Towers for the Experimental Simulation of Dust-aggregate Collisions in the Early Solar System

Laboratory Drop Towers for the Experimental Simulation of Dust-aggregate Collisions in the Early Solar System

Published on: June 5, 2014

Related Experiment Videos

Last Updated: May 21, 2026

Simulation of the Planetary Interior Differentiation Processes in the Laboratory

Simulation of the Planetary Interior Differentiation Processes in the Laboratory

Published on: November 15, 2013

Surface Mapping of Earth-like Exoplanets using Single Point Light Curves

Surface Mapping of Earth-like Exoplanets using Single Point Light Curves

Published on: May 10, 2020

Laboratory Drop Towers for the Experimental Simulation of Dust-aggregate Collisions in the Early Solar System

Laboratory Drop Towers for the Experimental Simulation of Dust-aggregate Collisions in the Early Solar System

Published on: June 5, 2014

Area of Science:

Exoplanetary Science
Planetary Dynamics
Astrobiology

Background:

The increasing number of known multi-planet systems provides a unique opportunity to study planetary formation and evolution.
Mean-motion resonances in planetary systems carry crucial information about their history and evolution.
Tidal interactions within gaseous discs drive planetary orbital migration during early system formation.

Purpose of the Study:

To present the observational properties of exoplanetary systems with confirmed or suspected resonant configurations.
To provide a comprehensive, updated list of known resonant systems for future research.
To facilitate the study of extrasolar system dynamics and test theoretical predictions.

Main Methods:

Observational data analysis of known multi-planet systems.
Identification and cataloging of systems exhibiting mean-motion resonances.
Comparative study of resonant configurations and their dynamical implications.

Main Results:

A complete list of known exoplanetary systems with resonant configurations is compiled.
The study highlights the significance of convergent differential migration in forming resonant captures.
Orbital migration during early formation is confirmed as a key factor in stable system architectures.

Conclusions:

Resonant configurations in exoplanetary systems are vital for understanding planet formation and evolution.
The cataloged resonant systems serve as a valuable reference for testing theories on planetary origins.
Studying these systems offers insights into the potential for life beyond Earth.