Led by Christopher Manser of the University of Warwick's Astrophysics Group, the researchers investigated the remnants of planetary systems
around white dwarf stars; in this instance, SDSS1228 +1040.
Not exact matches
The researchers found that relatively cool accretion discs
around young
stars, whose inner edges can be several times the size of the Sun, show the same behaviour as the hot, violent accretion discs
around planet - sized
white dwarfs, city - sized black holes and supermassive black holes as large as the entire Solar system, supporting the universality of accretion physics.
The small red circles denote other objects that emit X-rays, like neutron
stars or
white dwarfs, that are found scattered
around more of the galaxy.
Named PH1, the planet goes
around two of the four
stars, shown close - up here: One is a yellow -
white F - type
star that is slightly warmer and more luminous than our sun; the other, at the 11 o'clock position, is a red
dwarf, cooler and dimmer than the sun.
There are many
white dwarfs that hold large amounts of hydrogen in their atmospheres, and this new study suggests that this is evidence that water - rich asteroids or comets are common
around other
stars than the Sun.»
That is because
white dwarfs are 1000 times dimmer than
stars like the Sun, which are so bright that they overwhelm any reflected light from planets
around them.
As general relativity predicts, light from the background
star bent
around the
white dwarf, distorted by its gravitational field.
Previous work had unified the variability in discs
around black holes of different mass ranges, but by considering not just the mass of the object, but also its size, scientists can now add accreting
white dwarfs and proto -
stars to this unified picture.
The detected water most likely came from a minor planet, at least 90 km in diameter but probably much larger, that once orbited the GD 61
star before it became a
white dwarf around 200 million years ago.
Those remnants went into orbit
around the
white dwarf — much like the rings
around Saturn, Zuckerman said — before eventually spiraling onto the
star itself, bringing with them the building blocks for life.
As Vega is so much bigger and hotter than Sol, however, the
star will exhaust its core hydrogen after only another 650 million years or so (for a total life of
around a billion years) and turn into a red giant or Cepheid variable before puffing away its outer layers to reveal a remnant core as a
white dwarf.
HD 147513 A is a so - called young «Barium
dwarf» (s - process element rich but comparatively carbon deficient)
star that was probably enriched by an asymptotic branch giant (AGB)
star (see Gacrux) but is now a very dim,
white dwarf companion, which has an observed separation of
around 4,400 AUs — 5.7» at a HIPPARCOS distance estimate of 42.0 ly (Porto de Mello and da Silva, 1997; and Poveda et al, 1993, pp. 74 - 75).
the first debris disk
around a
star with a companion
white dwarf!
As US 708 traveled
around the
white dwarf, the dead
star would have stolen its helium.