Binary star formation

Binary star formation

R590/0146 Rights Managed

Request low-res file

530 pixels on longest edge, unwatermarked

Request/Download high-res file

Uncompressed file size: 50.6MB

Downloadable file size: 205.5KB

Price image Pricing

Please login to use the price calculator

This image is part of the sequence space: phases of a binary star formation
This image is part of the feature Dancing Newborn Stars


Caption: Binary star formation. Image 3 of 6. Supercomputer simulation of a pair of embryonic, or proto stars (white spots), forming in a molecular cloud core surrounded by spiralling clouds of gas (orange to red). Supercomputers help scientists understand how magnetic fields influence star formation. This simulation was run with the components interacting under a relatively low magnetic field. Under these conditions the gas cloud surrounding each molecular core is pulled by gravity to form two separate spirals. The system will eventually fragment to produce more stars. See images R590/144 to R590/149 for the full sequence. In simulations where the magnetic field is high binary stars collapse to form a single star. Simulation produced by Daniel Price, Exeter University, UK.

Release details: Model release not required. Property release not required.

Keywords: aggregating, astronomical, astronomy, astrophysical, astrophysics, binary star, binary stars, cosmology, couple, couples, daniel price, duo, evolution, exeter university, gas, interacting, interaction, low gravity, magnetic field, molecular cloud, pair, physics, proto star, protostar, science, space, spiral, spiralling, splash, star, star birth, starbirth, stars, stellar formation, supercomputer, supercomputer simulation, two, universe, visualisation sotware

Licence fees: A licence fee will be charged for any media (low or high resolution) used in your project.