Video Experimental Relacionado
Updated: Jul 11, 2026

11:34
Scattering And Absorption of Light in Planetary Regoliths
Published on: July 1, 2019
La mayoría de los meteoritos comunes encuentran un hogar entre los asteroides
Resumen
Los investigadores descubrieron que el asteroide tipo S Eros, orbitado por la nave espacial NEAR Shoemaker, comparte la misma composición elemental que las condritas ordinarias. Este hallazgo puede resolver el viejo rompecabezas de los orígenes de los meteoritos.
Área de la Ciencia:
- Ciencias planetarias Ciencias planetarias.
- Cosmoquímica es la cosmoquímica.
- La meteorología es meteorítica.
Sus antecedentes:
- Las condritas ordinarias son el tipo más común de meteorito que se encuentra en la Tierra.
- Los asteroides tipo S son el tipo más común de asteroides en el sistema solar interior.
- Un rompecabezas de larga data en la meteorítica es el aparente desajuste entre la composición de las condritas ordinarias y los asteroides de tipo S.
Objetivo del estudio:
- Para investigar la composición elemental del asteroide tipo S Eros.
- Para determinar si Eros tiene la misma composición que las condritas ordinarias.
- Para abordar la discrepancia entre los tipos comunes de meteoritos y los tipos comunes de asteroides.
Principales métodos:
- Análisis de la composición elemental utilizando datos de la nave espacial NEAR Shoemaker.
- Mediciones orbitales y in situ del asteroide Eros.
Principales resultados:
- El análisis de la nave espacial NEAR Shoemaker reveló que el asteroide Eros está compuesto de los mismos materiales que las condritas ordinarias.
- Esto marca el primer análisis de composición elemental de un asteroide realizado por una nave espacial.
Conclusiones:
- El asteroide tipo S Eros es una fuente potencial para meteoritos de condritas ordinarios.
- Este hallazgo ayuda a resolver el viejo rompecabezas sobre el origen de los meteoritos comunes.
- El análisis elemental basado en naves espaciales proporciona datos cruciales para comprender la formación y evolución del sistema solar.
Videos de Conceptos Relacionados
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,...
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 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...
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...
While in an elliptical orbit, the total energy of the planet is conserved. Therefore, the planet slows down when it is at apogee and...
Circular Orbits and Critical Velocity for Satellites
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...
Nicolaus Copernicus (1473-1543) first suggested that the Earth and all other planets orbit the Sun in...
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...
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...
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...
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...

