Jove
Visualize
Contáctanos

Videos de Conceptos Relacionados

Atomic Structure01:33

Atomic Structure

All matter is composed of atoms, the smallest individual units of elements. Each atom is made up of three subatomic particles: protons, neutrons, and electrons. Together, these three particles account for the mass and the charge of an atom.The History of Atomic TheoryThe first person to propose that everything on Earth is made up of tiny particles was the Greek philosopher Democritus, around 450 B.C. He used the term atomos, Greek for “indivisible,” from which the modern term “atom” is derived.
Conditions on Early Earth02:06

Conditions on Early Earth

Around 4 billion years ago, oceans began to condense on earth while volcanic eruptions released nitrogen, carbon dioxide, methane, ammonia, and hydrogen into the primordial atmosphere. However, organisms with the characteristics of life were not initially present on earth. Scientists have used experimentation to determine how organisms evolved that could grow, reproduce, and maintain an internal environment.
Subatomic Particles03:37

Subatomic Particles

Dalton was only partially correct about the particles that make up matter. All matter is composed of atoms, and atoms are composed of three smaller subatomic particles: protons, neutrons, and electrons. These three particles account for the mass and the charge of an atom.
Constant Volume Calorimetry02:41

Constant Volume Calorimetry

Calorimeters are useful to determine the heat released or absorbed by a chemical reaction. Coffee cup calorimeters are designed to operate at constant (atmospheric) pressure and are convenient to measure heat flow (or enthalpy change) accompanying processes that occur in solution at constant pressure. A different type of calorimeter that operates at constant volume, colloquially known as a bomb calorimeter, is used to measure the energy produced by reactions that yield large amounts of heat and...
Conditions on Early Earth02:06

Conditions on Early Earth

Around 4 billion years ago, oceans began to condense on earth while volcanic eruptions released nitrogen, carbon dioxide, methane, ammonia, and hydrogen into the primordial atmosphere. However, organisms with the characteristics of life were not initially present on earth. Scientists have used experimentation to determine how organisms evolved that could grow, reproduce, and maintain an internal environment.
Atomic Structure01:17

Atomic Structure

The Greek philosopher Democritus proposed that everything on Earth is made up of tiny particles called atomos, Greek for "indivisible," from which the modern term "atom" is derived. In the 19th century, John Dalton proposed the atomic theory that is still largely correct today. He put forth five postulates to explain how atoms made up the world around us. (1) All matter is composed of infinitely small particles or atoms. (2) All atoms of a given element are identical to one another and (3) are...

También podría leer

Artículos Relacionados

Artículos vinculados a este trabajo por autores compartidos, revista y gráfico de citas.

Ordenar por
Same author

National Meat Case Study 2004: Product labeling information, branding, and packaging trends.

Journal of animal science·2008
Same author

National Meat Case Study 2004: Fresh product types and allocation of retail space.

Journal of animal science·2008
Same author

TELESCOPES: Astronomers Overcome 'Aperture Envy'.

Science (New York, N.Y.)·2007
Same author

KIP THORNE: The Shaman of Space and Time.

Science (New York, N.Y.)·2007
Same author

AAS HIGH-ENERGY ASTROPHYSICS DIVISION: X-rays Hit the Spot for Astrophysicists.

Science (New York, N.Y.)·2007
Same author

AMERICAN ASTRONOMICAL SOCIETY MEETING: Cool Comets, Barren Clusters, and a Maxed-Out Universe.

Science (New York, N.Y.)·2007
JoVE
x logofacebook logolinkedin logoyoutube logo
ACERCA DE JoVE
Visión GeneralLiderazgoBlogCentro de Ayuda JoVE
AUTORES
Proceso de PublicaciónConsejo EditorialAlcance y PolíticasRevisión por ParesPreguntas FrecuentesEnviar
BIBLIOTECARIOS
TestimoniosSuscripcionesAccesoRecursosConsejo Asesor de BibliotecasPreguntas Frecuentes
INVESTIGACIÓN
JoVE JournalMethods CollectionsJoVE Encyclopedia of ExperimentsArchivo
EDUCACIÓN
JoVE CoreJoVE BusinessJoVE Science EducationJoVE Lab ManualCentro de Recursos para ProfesoresSitio de Profesores
Términos y Condiciones de Uso
Política de Privacidad
Políticas

Video Experimental Relacionado

Updated: Jul 9, 2026

A Method for Studying the Temperature Dependence of Dynamic Fracture and Fragmentation
09:12

A Method for Studying the Temperature Dependence of Dynamic Fracture and Fragmentation

Published on: June 28, 2015

ASTRÓFÍSICA: Los astrónomos detectan su primera bomba de carbono.

R Irion

    Science (New York, N.Y.)
    |September 6, 2007
    PubMed
    Resumen
    Este resumen es generado por máquina.

    Una explosión termonuclear alimentada con carbono en una estrella ultradensa.

    Más Videos Relacionados

    Preparation and Reactivity of Gasless Nanostructured Energetic Materials
    09:50

    Preparation and Reactivity of Gasless Nanostructured Energetic Materials

    Published on: April 2, 2015

    Blast Quantification Using Hopkinson Pressure Bars
    09:41

    Blast Quantification Using Hopkinson Pressure Bars

    Published on: July 5, 2016

    Videos de Experimentos Relacionados

    Last Updated: Jul 9, 2026

    A Method for Studying the Temperature Dependence of Dynamic Fracture and Fragmentation
    09:12

    A Method for Studying the Temperature Dependence of Dynamic Fracture and Fragmentation

    Published on: June 28, 2015

    Preparation and Reactivity of Gasless Nanostructured Energetic Materials
    09:50

    Preparation and Reactivity of Gasless Nanostructured Energetic Materials

    Published on: April 2, 2015

    Blast Quantification Using Hopkinson Pressure Bars
    09:41

    Blast Quantification Using Hopkinson Pressure Bars

    Published on: July 5, 2016

    Área de la Ciencia:

    • La astrofísica es la astrofísica.
    • Evolución Estelar Evolución Estelar

    Sus antecedentes:

    • Las explosiones termonucleares en las estrellas suelen involucrar hidrógeno o helio.
    • Comprender la combustión estelar es clave para la astrofísica.

    Objetivo del estudio:

    • Para informar sobre el posible descubrimiento de una explosión estelar termonuclear de solo carbono.
    • Para investigar las implicaciones para los modelos estelares.

    Principales métodos:

    • Observación de un evento de explosión cósmica.
    • Análisis de la composición elemental de la explosión.

    Principales resultados:

    • Una explosión termonuclear de 3 horas en la superficie de una estrella ultradensa.
    • La explosión parece ser alimentada únicamente por el carbono.

    Conclusiones:

    • Este evento podría ser la primera explosión cósmica observada impulsada exclusivamente por el carbono.
    • La confirmación puede llevar a revisiones en los modelos de combustión estelar y detonación de carbono.