Jove
Visualize
Contact Us

Related Concept Videos

Precipitate Formation and Particle Size Control01:16

Precipitate Formation and Particle Size Control

947
In precipitation gravimetry, the precipitating agent should react specifically or selectively with the analyte. While a specific reagent reacts with the analyte alone, a selective reagent can react with a limited number of chemical species.
The obtained precipitate should be either a pure substance of known composition or easily converted to one by a simple process, such as ignition or drying. In addition, the precipitate should be insoluble and easily filterable. In general, filterability...
947
Conditions on Early Earth02:06

Conditions on Early Earth

96.4K
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.
96.4K
Phase Transitions: Sublimation and Deposition02:33

Phase Transitions: Sublimation and Deposition

17.9K
Some solids can transition directly into the gaseous state, bypassing the liquid state, via a process known as sublimation. At room temperature and standard pressure, a piece of dry ice (solid CO2) sublimes, appearing to gradually disappear without ever forming any liquid. Snow and ice sublimate at temperatures below the melting point of water, a slow process that may be accelerated by winds and the reduced atmospheric pressures at high altitudes. When solid iodine is warmed, the solid sublimes...
17.9K
Solution Formation02:16

Solution Formation

32.7K
There is no one solvent that can dissolve every type of solute. Some substances that readily dissolve in a certain solvent might be insoluble in a different solvent. A simple way to predict which substances dissolve in which solvent is the phrase "like dissolves like". This means that polar substances, such as salt and sugar, dissolve in a polar substance like water. In contrast, non-polar substances are more soluble in non-polar solvents such as carbon tetrachloride.
This selective...
32.7K
Formation of Complex Ions03:45

Formation of Complex Ions

24.0K
A type of Lewis acid-base chemistry involves the formation of a complex ion (or a coordination complex) comprising a central atom, typically a transition metal cation, surrounded by ions or molecules called ligands. These ligands can be neutral molecules like H2O or NH3, or ions such as CN− or OH−. Often, the ligands act as Lewis bases, donating a pair of electrons to the central atom. These types of Lewis acid-base reactions are examples of a broad subdiscipline called coordination...
24.0K
Elastic Collisions: Introduction01:00

Elastic Collisions: Introduction

13.1K
An elastic collision is one that conserves both internal kinetic energy and momentum. Internal kinetic energy is the sum of the kinetic energies of the objects in a system. Truly elastic collisions can only be achieved with subatomic particles, such as electrons striking nuclei. Macroscopic collisions can be very nearly, but not quite, elastic, as some kinetic energy is always converted into other forms of energy such as heat transfer due to friction and sound. An example of a nearly...
13.1K
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
  1. Home
  2. Chondrule Formation By Collisions Of Planetesimals Containing Volatiles Triggered By Jupiter's Formation.
  1. Home
  2. Chondrule Formation By Collisions Of Planetesimals Containing Volatiles Triggered By Jupiter's Formation.

Related Experiment Video

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

12.9K

Chondrule formation by collisions of planetesimals containing volatiles triggered by Jupiter's formation.

Sin-Iti Sirono1, Diego Turrini2

  • 1Graduate School of Earth and Environmental Sciences, Nagoya University, Nagoya, Japan. sirono@eps.nagoya-u.ac.jp.

Scientific Reports
|August 25, 2025

View abstract on PubMed

Summary
This summary is machine-generated.

Collisions between planetesimals containing volatile materials explain chondrule formation. Jupiter's formation triggered these impacts, producing silicate melt dispersed by gas, matching chondrule sizes and cooling rates.

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

11.7K
Metal-silicate Partitioning at High Pressure and Temperature: Experimental Methods and a Protocol to Suppress Highly Siderophile Element Inclusions
11:50

Metal-silicate Partitioning at High Pressure and Temperature: Experimental Methods and a Protocol to Suppress Highly Siderophile Element Inclusions

Published on: June 13, 2015

12.6K

Related Experiment Videos

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

12.9K
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

11.7K
Metal-silicate Partitioning at High Pressure and Temperature: Experimental Methods and a Protocol to Suppress Highly Siderophile Element Inclusions
11:50

Metal-silicate Partitioning at High Pressure and Temperature: Experimental Methods and a Protocol to Suppress Highly Siderophile Element Inclusions

Published on: June 13, 2015

12.6K

Area of Science:

  • Planetary Science
  • Cosmochemistry
  • Astrophysics

Background:

  • Chondrules are key components of chondritic meteorites, providing insights into early solar system processes.
  • Observed chondrule sizes and cooling rates are difficult to reconcile with existing formation models.
  • Understanding chondrule formation is crucial for dating the early solar system and understanding planet formation.

Purpose of the Study:

  • To propose and numerically validate a new model for chondrule formation.
  • To explain the characteristic sizes and cooling rates of chondrules.
  • To link chondrule formation to the early stages of Jupiter's formation and the solar nebula.

Main Methods:

  • Numerical simulations of high-velocity planetesimal collisions.
  • Modeling of silicate melt generation and dispersal by volatile-driven gas expansion.
  • Analysis of melt production rates linked to Jupiter's gas accretion.
  • Main Results:

    • High-velocity collisions (>2 km/s) of volatile-rich planetesimals generate significant silicate melt.
    • Expanding gas from heated volatiles disperses and cools the melt, forming chondrule-sized droplets.
    • Peak melt production correlates with the onset of Jupiter's runaway gas accretion.

    Conclusions:

    • Planetesimal collisions provide a natural mechanism for chondrule formation, explaining their observed properties.
    • Chondrule formation provides a temporal marker, suggesting Jupiter formed approximately 1.8 Myr after Calcium-Aluminum-rich Inclusions (CAIs).
    • This model reconciles chondrule characteristics with early solar system dynamics and Jupiter's formation timeline.