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

Intermolecular Forces03:13

Intermolecular Forces

Atoms and molecules interact through bonds (or forces): intramolecular and intermolecular. The forces are electrostatic as they arise from interactions (attractive or repulsive) between charged species (permanent, partial, or temporary charges) and exist with varying strengths between ions, polar, nonpolar, and neutral molecules. The different types of intermolecular forces are ion–dipole, dipole–dipole, hydrogen bonds, and dispersion; among these, dipole–dipole, hydrogen bonds, and dispersion...
Intermolecular Forces03:13

Intermolecular Forces

Atoms and molecules interact through bonds (or forces): intramolecular and intermolecular. The forces are electrostatic as they arise from interactions (attractive or repulsive) between charged species (permanent, partial, or temporary charges) and exist with varying strengths between ions, polar, nonpolar, and neutral molecules. The different types of intermolecular forces are ion–dipole, dipole–dipole, hydrogen bonds, and dispersion; among these, dipole–dipole, hydrogen bonds, and dispersion...
Behavior of Gas Molecules: Molecular Diffusion, Mean Free Path, and Effusion03:48

Behavior of Gas Molecules: Molecular Diffusion, Mean Free Path, and Effusion

Although gaseous molecules travel at tremendous speeds (hundreds of meters per second), they collide with other gaseous molecules and travel in many different directions before reaching the desired target. At room temperature, a gaseous molecule will experience billions of collisions per second. The mean free path is the average distance a molecule travels between collisions. The mean free path increases with decreasing pressure; in general, the mean free path for a gaseous molecule will be...
Real Gases: Effects of Intermolecular Forces and Molecular Volume Deriving Van der Waals Equation04:01

Real Gases: Effects of Intermolecular Forces and Molecular Volume Deriving Van der Waals Equation

Thus far, the ideal gas law, PV = nRT, has been applied to a variety of different types of problems, ranging from reaction stoichiometry and empirical and molecular formula problems to determining the density and molar mass of a gas. However, the behavior of a gas is often non-ideal, meaning that the observed relationships between its pressure, volume, and temperature are not accurately described by the gas laws.
Molecular Orbital Theory II03:51

Molecular Orbital Theory II

Molecular Orbital Energy Diagrams
Molecular Orbital Theory I02:35

Molecular Orbital Theory I

Overview of Molecular Orbital Theory

You might also read

Related Articles

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

Sort by
Same author

Bis-Dichlorosilyl Functionalized C<sub>4</sub>-Cumulene With Unique Bonding Scenario.

Chemistry (Weinheim an der Bergstrasse, Germany)·2026
Same author

Valorization of CO<sub>2</sub> and N<sub>2</sub>O Gas Enabled by a Single Multi-Photoinduced Electron Transfer Catalyst.

Journal of the American Chemical Society·2025
Same author

Mesoionic N-Heterocyclic Olefins, Imines, Thiones, Phosphinidenes and Their Application in Catalysis.

Angewandte Chemie (International ed. in English)·2025
Same author

Redox Umpolung of Phenalenyl-Based Molecule Inside Water-Soluble Nanocages.

Journal of the American Chemical Society·2025
Same author

Coordination Chemistry of Phosphinidene Stabilized by Mesoionic N-heterocyclic Carbene and Catalysis.

Chemistry (Weinheim an der Bergstrasse, Germany)·2025
Same author

Bifunctional Silylene-Aminoborane Enables Cooperative Activation of Unsaturated Bonds and Access to Heteroatom-Enriched Polycycle.

Angewandte Chemie (International ed. in English)·2025

Related Experiment Video

Updated: Jun 10, 2026

Spatial Separation of Molecular Conformers and Clusters
10:37

Spatial Separation of Molecular Conformers and Clusters

Published on: January 9, 2014

Interstellar molecules: guides for new chemistry.

Swadhin K Mandal1, Herbert W Roesky

  • 1Department of Chemical Sciences, Indian Institute of Science Education and Research-Kolkata, Mohanpur-741252, India. swadhin.mandal@iiserkol.ac.in

Chemical Communications (Cambridge, England)
|July 28, 2010
PubMed
Summary

Researchers synthesized unstable low-valent main group elements, mimicking interstellar conditions. Sterically protected ligands prevent disproportionation, enabling the study of these rare molecules in the lab.

More Related Videos

Coulomb Explosion Imaging as a Tool to Distinguish Between Stereoisomers
08:51

Coulomb Explosion Imaging as a Tool to Distinguish Between Stereoisomers

Published on: August 18, 2017

Combustion Chemistry of Fuels: Quantitative Speciation Data Obtained from an Atmospheric High-temperature Flow Reactor with Coupled Molecular-beam Mass Spectrometer
07:24

Combustion Chemistry of Fuels: Quantitative Speciation Data Obtained from an Atmospheric High-temperature Flow Reactor with Coupled Molecular-beam Mass Spectrometer

Published on: February 19, 2018

Related Experiment Videos

Last Updated: Jun 10, 2026

Spatial Separation of Molecular Conformers and Clusters
10:37

Spatial Separation of Molecular Conformers and Clusters

Published on: January 9, 2014

Coulomb Explosion Imaging as a Tool to Distinguish Between Stereoisomers
08:51

Coulomb Explosion Imaging as a Tool to Distinguish Between Stereoisomers

Published on: August 18, 2017

Combustion Chemistry of Fuels: Quantitative Speciation Data Obtained from an Atmospheric High-temperature Flow Reactor with Coupled Molecular-beam Mass Spectrometer
07:24

Combustion Chemistry of Fuels: Quantitative Speciation Data Obtained from an Atmospheric High-temperature Flow Reactor with Coupled Molecular-beam Mass Spectrometer

Published on: February 19, 2018

Area of Science:

  • Astrochemistry
  • Main Group Chemistry

Background:

  • Interstellar space hosts unique chemical environments with unstable low-valent main group elements.
  • Carbon and silicon in low-valent states are observed in the interstellar medium, prompting laboratory investigation.

Purpose of the Study:

  • To explore the synthesis of unstable molecules containing heavier low-valent Group 14 elements.
  • To investigate methods for stabilizing these species, inspired by interstellar chemistry.

Main Methods:

  • Utilizing sterically protected ligands to control reactivity.
  • Investigating the disproportionation pathways of low-valent Group 14 elements.

Main Results:

  • Demonstrated the successful arrest of the disproportionation pathway for heavier low-valent Group 14 elements.
  • Developed a laboratory method to generate conditions mimicking the dilute, stable environment of interstellar molecules.

Conclusions:

  • Sterically protected ligands are effective in stabilizing reactive low-valent main group elements.
  • This approach allows for the laboratory study of species relevant to interstellar astrochemistry.