An artist's conception of PSR 1257+12's system of planets Pulsars are rapidly rotating neutron stars. Pulsar planets are planets that are found orbiting pulsars. The first such planet to be discovered was around a millisecond pulsar. Pulsar planets are discovered through pulsar timing measurements, to detect anomalies in the pulsation period. Any bodies orbiting the pulsar will cause regular changes in its pulsation. Since pulsars normally rotate at near-constant speed, any changes can easily be detected with the help of precise timing measurements. Image File history File linksMetadata Download high resolution version (3000x2400, 2719 KB) Summary Licensing File history Legend: (cur) = this is the current file, (del) = delete this old version, (rev) = revert to this old version. ...
Image File history File linksMetadata Download high resolution version (3000x2400, 2719 KB) Summary Licensing File history Legend: (cur) = this is the current file, (del) = delete this old version, (rev) = revert to this old version. ...
PSR 1257+12 (also catalogued as PSR B1257+12, PSR 1300+1240, or PSR J1300+1240) is a pulsar located 980 light years from Earth. ...
A neutron star is one of the few possible endpoints of stellar evolution. ...
Composite Optical/X-ray image of the Crab Nebula pulsar, showing surrounding nebular gases stirred by the pulsars magnetic field and radiation. ...
An extrasolar planet, or exoplanet, is a planet beyond the Solar System. ...
A millisecond pulsar (MSP), often referred to as recycled pulsar, is a pulsar with a rotational period in the range of about 1-10 milliseconds. ...
In 2006 the pulsar 4U 0142+61, located 13,000 light years from Earth, was found to have a circumstellar disk. The discovery was made by a team led by Deepto Chakrabarty of MIT using the Spitzer Space Telescope.[1] The disk is thought to have formed from metal-rich debris left over from the supernova that formed the pulsar roughly 100,000 years ago and is similar to those seen around Sun-like stars, suggesting it may be capable of forming planets in a similar fashion. Pulsar planets would be entirely incapable of supporting any form of life as we know it due to the colossal amounts of electromagnetic radiation emitted by pulsars. 2006 (MMVI) is a common year starting on Sunday of the Gregorian calendar. ...
4U 0142+61 is a magnetar at an approximate distance of 13,000 ly from Earth, located in the constellation Cassiopeia. ...
A protoplanetary disc (also protoplanetary disk, proplyd) is an accretion disc surrounding a T Tauri star. ...
Mapúa Institute of Technology (MIT, MapúaTech or simply Mapúa) is a private, non-sectarian, Filipino tertiary institute located in Intramuros, Manila. ...
The Spitzer Space Telescope Facility launches from Cape Canaveral Air Force Station in Florida on Monday, Aug. ...
Multiwavelength X-ray image of the remnant of Keplers Supernova, SN 1604. ...
List of known pulsar planets Confirmed planets | Pulsar | Planet | Mass | | PSR B1620-26 | PSR B1620-26c | 2.5 MJ | | PSR 1257+12 | PSR 1257+12 A | 0.020 ME | | PSR 1257+12 B | 4.3 ME | | PSR 1257+12 C | 3.90 ME | | PSR 1257+12 D | 0.0004 ME | Unsolved problems in physics: What causes anything to have mass? Mass is a property of a physical object that quantifies the amount of matter and energy it is equivalent to. ...
PSR B1620-26 is also called PSR J1623-2631 (or or ) // System Configuration PSR B1620-26 is a pulsar in the globular cluster Messier 4 (or M4: see Messier object), about 5,600 light years from Earth in the constellation Scorpius. ...
An artists impression of the view from near the planet PSR B1620-26c is a planet orbiting the pulsar PSR B1620-26 in the globular cluster Messier 4, about 12,400 light years from Earth in the constellation of Scorpius. ...
PSR 1257+12 (also catalogued as PSR B1257+12, PSR 1300+1240, or PSR J1300+1240) is a pulsar located 980 light years from Earth. ...
Doubtful planets | Pulsar | Planet | Mass | | Geminga | Geminga b | 1.7 ME | | PSR B0329+54 | PSR B0329+54 A | 0.3 ME | | PSR B0329+54 B | 2.2 ME | | PSR B1828-10 | PSR B1828-10 A | 3 ME | | PSR B1828-10 B | 12 ME | | PSR B1828-10 C | 8 ME | Unsolved problems in physics: What causes anything to have mass? Mass is a property of a physical object that quantifies the amount of matter and energy it is equivalent to. ...
Geminga (Gemini gamma-ray source) is a neutron star approximately 552 light-years away in the constellation Gemini. ...
Proplyds 4U 0142+61 is a magnetar at an approximate distance of 13,000 ly from Earth, located in the constellation Cassiopeia. ...
See also The following are lists of stars with confirmed extrasolar planets. ...
This is a list of unconfirmed extrasolar planets. ...
This is a list of protoplanetary discs. ...
An extrasolar planet, or exoplanet, is a planet beyond the Solar System. ...
Andrew G. Lyne (born 1942) is a British physicist. ...
Aleksander Wolszczan (b. ...
Dale Frail is an astronomer. ...
References - ^ Scientists crack mystery of planet formation. CNN.com (April 5, 2006). Retrieved on 2006-04-05.
‹The stub template below has been proposed for renaming to extrasolar-planet-stub. See stub types for deletion to help reach a consensus on what to do.› |