Қайталанатын жаңа жұлдыз - T Pyxidis

Recurrent nova star in the constellation Pyxis

Starbox catalog
| names = is a recurrent nova
and nova remnant in the constellation Pyxis. It is a binary star system and its distance is estimated at from Earth. It contains a Sun like star and a white dwarf. Because of their close proximity and the larger mass of the white dwarf, the latter draws matter from the larger, less massive star. The influx of matter on the white dwarf's surface causes periodic thermonuclear explosions to occur. The usual apparent magnitude of this star system is 15.5, but there have been observed eruptions with maximal apparent magnitude of about 7.0 in the years 1890, 1902, 1920, 1944, 1966 and 2011. Evidence seems to indicate that T Pyxidis may have increased in mass despite the nova eruptions, and is now close to the Chandrasekhar limit when it might explode as a supernova. When a white dwarf reaches this limit it will collapse under its own weight and cause a type Ia supernova.

Because of its relative proximity, some—in particular, Edward Sion, astronomer & astrophysicist at Villanova University, and his team therefrom—contend that a type 1a supernova could have a significant impact on Earth. The received gamma radiation would equal the total (all spectra) radiation of approximately 1,000 solar flares, but the type Ia supernova would have to be closer than to cause significant damage to the ozone layer, and perhaps closer than 500 parsecs. The X radiation that reaches Earth in such an event, however, would be less than the X radiation of a single average solar flare. Mankind survived when the radiation from the Crab Nebula supernova, at a distance of about 6,500 light years, reached Earth in the year 1054. A type Ia supernova at a distance of 3,300 light years would have an apparent magnitude of around 9.3, about as bright as the brightest Iridium (satellite) flares. Recent data indicates his distance estimate is five times too close. Astronomers used NASA's Hubble Space Telescope to observe the light emitted during its latest outburst in April 2011. The team also used the light echo to refine estimates of the nova's distance from Earth. The new distance is 15,600 light years (4780 pc) from Earth. Previous estimates were between 6,500 and 16,000 light years (2000 and 4900 pc). It has been reported that T Pyx would "soon" become a supernova. By that time it will have moved far enough away from the Solar System to have little effect.

Mike Linnolt detected T Pyx's first outburst in nearly 45 years on April 14, 2011, at magnitude 13. According to AAVSO observers, it reached magnitude 7.5 in the visual and V bands by April 27, and reached magnitude 6.8 by May 3.

T Pyxidis is a super soft X ray source.