PSR J1719−1438

Diamond planet

Main article: PSR J1719−1438 b

PSR J1719−1438 was discovered in 2011 by the High Time Resolution Survey, a radio astronomy search for astronomical objects that rapidly vary in radio brightness, such as pulsars. Timing measurements using the Parkes Telescope and Lovell Telescope showed that it has a low-mass companion: PSR J1719−1438 b. The companion has a mass similar to that of Jupiter, but 40% of the diameter. It orbits the pulsar with a period of 2 hours 10 minutes and 37 seconds, at a distance of around 600,000 km (0.89 solar radii). The companion is likely the remnant of a star whose outer layers were siphoned off by the more massive pulsar. Calculations show the companion has a minimum density of 23 grams per cubic centimeter and is probably an ultra-low-mass carbon–oxygen white dwarf.

Because the companion to PSR J1719−1438 is planet-sized, made primarily of carbon (with an unknown amount of oxygen), and very dense, it may be similar to a large diamond. In the science press, the object has been called the "Diamond Planet".

A lump of QCD matter

It has been suggested in 2012 that PSR J1719−1438 b may not be the remnant of a white dwarf, but a lump of quark matter with a size of just 1 kilometer and the mass of Jupiter, that would have been born in the collision and merger of two previous quark stars, part of the ejected matter ending orbiting the merger remnant we see as the pulsar PSR J1719−1438.

References

References

1. {{cite constellation. PSR J1719-1438
2. Tillman, Nola Taylor. (August 25, 2011). "Surprise! Alien Planet Made of Diamond Discovered". [[Space.com]].
3. van Haaften, L. M.. "Formation of the planet around the millisecond pulsar J1719–1438".
4. (25 August 2011). "Star Transforms into A Diamond Planet". Universe Today.
5. (25 August 2011). "Surprise! Alien Planet Made of Diamond Discovered". Space.com.
6. "A Planet made of Diamond". Max Planck Institut for Radio Astronomy.