Jove
Visualize
Contact Us
JoVE
x logofacebook logolinkedin logoyoutube logo
ABOUT JoVE
OverviewLeadershipBlogJoVE Help Center
AUTHORS
Publishing ProcessEditorial BoardScope & PoliciesPeer ReviewFAQSubmit
LIBRARIANS
TestimonialsSubscriptionsAccessResourcesLibrary Advisory BoardFAQ
RESEARCH
JoVE JournalMethods CollectionsJoVE Encyclopedia of ExperimentsArchive
EDUCATION
JoVE CoreJoVE BusinessJoVE Science EducationJoVE Lab ManualFaculty Resource CenterFaculty Site
Terms & Conditions of Use
Privacy Policy
Policies

Related Concept Videos

Acceleration due to Gravity on Other Planets01:24

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...
Acceleration due to Gravity on Earth00:55

Acceleration due to Gravity on Earth

Newton's second law is closely related to his first law of motion. It mathematically gives the cause-and-effect relationship between force and changes in motion. Newton's second law is quantitative and is used extensively to calculate what happens in situations involving a force. All external forces acting on a system add together to produce a net force Fnet. A larger net external force produces a larger acceleration. This acceleration is directly proportional to, and in the same direction as,...
Acceleration due to Gravity on Earth01:21

Acceleration due to Gravity on Earth

According to Newton's law of gravitation, the gravitational force on a body is proportional to its mass. According to Newton's second law of motion, the acceleration produced by an external force is inversely proportional to the force. Hence, the acceleration of an object under an external force of gravitation is independent of its mass.
The acceleration of an object close to the Earth, because of the Earth's gravitational pull, is called the acceleration due to gravity. It is always directed...
Gravity between Spherical Bodies01:27

Gravity between Spherical Bodies

Newton's law of gravitation describes the gravitational force between any two point masses. However, for extended spherical objects like the Earth, the Moon, and other planets, the law holds with an assumption that masses of spherical objects are concentrated at their respective centers.
This assumption can be proved easily by showing that the expression for gravitational potential energy between a hollow sphere of mass (M) and a point mass (m) is the same as it would be for a pair of extended...
Newton's Law of Gravitation01:15

Newton's Law of Gravitation

Our everyday observation tells us that all objects close to the Earth naturally tend to fall to the ground. Early philosophers assumed that this downward force was unique to Earth. By the 16th century, Nicolaus Copernicus (1473-1543) put forward the heliocentric theory, which suggested that Earth and other planets orbited the sun, while the Moon orbited the Earth. However, it was Isaac Newton (1642-1727) who linked these two motions together in the 17th century. He reasoned that the force of...
Rocket Propulsion in Gravitational Field - II01:03

Rocket Propulsion in Gravitational Field - II

A rocket's velocity in the presence of a gravitational field is decreased by the amount of force exerted by Earth's gravitational field, which opposes the motion of the rocket. If we consider thrust, that is, the force exerted on a rocket by the exhaust gases, then a rocket's thrust is greater in outer space than in the atmosphere or on a launch pad. In fact, gases are easier to expel in a vacuum.
A rocket's acceleration depends on three major factors, consistent with the equation for the...

You might also read

Related Articles

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

Sort by
Same author

Nucleation experiments on a titanium-carbon system imply nonclassical formation of presolar grains.

Science advances·2023
Same author

TEMPus VoLA: The timed Epstein multi-pressure vessel at low accelerations.

The Review of scientific instruments·2022
Same author

The Philae lander reveals low-strength primitive ice inside cometary boulders.

Nature·2020
Same journal

Erratum: "Highly versatile, two-color setup for high-order harmonic generation using spatial light modulators" [Rev. Sci. Instrum. 95, 073002 (2024)].

The Review of scientific instruments·2026
Same journal

Thermal correction method for accurate performance evaluation of micro-thermoelectric coolers.

The Review of scientific instruments·2026
Same journal

Correcting the energy-dependent asymmetry in low-energy muon spin rotation.

The Review of scientific instruments·2026
Same journal

Fiber-integrated acousto-optic-modulator-based phase-controlled Rydberg atomic electrometer.

The Review of scientific instruments·2026
Same journal

A top-loading point-contact spectroscopy probe with in-situ sample exchange for dilution refrigerators.

The Review of scientific instruments·2026
Same journal

Investigation of plasma characteristics in a developed large-diameter, low-aspect ratio, radio frequency plasma source with a flat spiral antenna.

The Review of scientific instruments·2026
See all related articles

Related Experiment Video

Updated: May 28, 2026

Laboratory Drop Towers for the Experimental Simulation of Dust-aggregate Collisions in the Early Solar System
09:44

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

Published on: June 5, 2014

A simulation platform for small solar system bodies' gravity using the Einstein-Elevator.

E Tahtali1, C Kreuzig2, G Meier2

  • 1Leibniz University Hannover, Institute of Transport and Automation Technology, An der Universitaet 2, 30823 Garbsen, Germany.

The Review of Scientific Instruments
|May 26, 2026
PubMed
Summary
This summary is machine-generated.

Researchers developed a novel system to simulate partial gravity conditions for small solar system bodies (SSSBs) like asteroids and comets on Earth. This breakthrough enables studying SSSB behavior under controlled, low-gravity environments, advancing space exploration research.

More Related Videos

Simulation of the Planetary Interior Differentiation Processes in the Laboratory
06:04

Simulation of the Planetary Interior Differentiation Processes in the Laboratory

Published on: November 15, 2013

Experimental Methods for Efficient Solar Hydrogen Production in Microgravity Environment
11:38

Experimental Methods for Efficient Solar Hydrogen Production in Microgravity Environment

Published on: December 3, 2019

Related Experiment Videos

Last Updated: May 28, 2026

Laboratory Drop Towers for the Experimental Simulation of Dust-aggregate Collisions in the Early Solar System
09:44

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

Published on: June 5, 2014

Simulation of the Planetary Interior Differentiation Processes in the Laboratory
06:04

Simulation of the Planetary Interior Differentiation Processes in the Laboratory

Published on: November 15, 2013

Experimental Methods for Efficient Solar Hydrogen Production in Microgravity Environment
11:38

Experimental Methods for Efficient Solar Hydrogen Production in Microgravity Environment

Published on: December 3, 2019

Area of Science:

  • Planetary Science
  • Astrophysics
  • Space Engineering

Background:

  • Small solar system bodies (SSSBs), including asteroids and comets, are crucial for understanding planetary formation and evolution.
  • Studying SSSBs on Earth is challenging due to the difficulty in simulating their low-gravity environments.
  • Missions like OSIRIS-REx and Rosetta highlight the increasing importance of SSSB research.

Purpose of the Study:

  • To develop and validate a method for simulating partial gravity conditions (10^-2 to 10^-4g) for SSSBs on Earth.
  • To enable the study of SSSB characteristics and behavior under controlled, simulated low-gravity environments.
  • To provide a proof of concept for adjustable gravity generation in drop tower facilities.

Main Methods:

  • An acceleration system using servo motors and spindle axes was designed to simulate partial gravity.
  • A comet-like sample was subjected to accelerations within a vacuum chamber (10^-6 mbar).
  • The setup was installed and tested within the Einstein-Elevator facility.

Main Results:

  • The system successfully generated gravity levels from 10^-2g down to 10^-3g.
  • Maximum deviations during acceleration were ±5 x 10^-4g.
  • Experiment durations of at least 2.5 seconds were achieved at 10^-2g, with a planned minimum of 3.5 seconds at 10^-4g.

Conclusions:

  • The developed system effectively simulates partial gravity conditions relevant to SSSBs.
  • This approach provides a viable method for conducting SSSB experiments on Earth.
  • The proof of concept paves the way for future research into SSSB activity under simulated partial gravity.