News on Exoplanets
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- First direct ligth from Earthlike exoplanet
- Look for Jupiter-like planets, when you search for Earth-like planets
- Stars occasionally capture wandering planets
- Discovery of two planetary babies
- New study suggests the Solarsystem is the norm
- A star with 9 exoplanets
- Discovery of 2 very old exoplanets
- Millions of Earthlike planets in th eMilkyway
- Premature planetary-formation
- Runaway planets
- Kepler releases new catalog-2321 planet candidates
- Water in the atmosphere of a super-Earth
- New 3D model for planetary accretion
- Red dwarf stars may be more habitable than imagined
- Our galaxy may swarm with free--floating planets
- Hubble reveals a new class of exoplanet
- Discovery of potential habitable exoplanet
- 11 new solarsystems hosting 26 planets discovered
- First SETI observations of Kepler candidates
- Discovery of smallest known exoplanets
- New class of planetary system
- Searching for habitable exo-moons
- Discovery of 2 Earth-size planets raises questions about stellar evolution
- Kepler discovers first truly Earth-sized planets
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Can life survive around a white dwarf star?
Wednesday, 23 March 2011 11:04
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| Astronomy - Exoplanets |
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In 5-6 biollion years the Sun will end its life as a white dwarf-star, just as most other main-sequence stars. But can a white dwarf support life?
A white dwarf, also called a degenerate dwarf, is a small star composed mostly of electron-degenerate matter. They are very dense; a white dwarf's mass is comparable to that of the Sun and its volume is comparable to that of the Earth. Its faint luminosity comes from the emission of stored thermal energy. In January 2009, the Research Consortium on Nearby Stars project counted eight white dwarfs among the hundred nearest star systems of the Sun. To date the search for habitable Earth-like planets has primarily focused on nuclear burning stars. This research propose that this search should be expanded to cool white dwarf stars that have expended their nuclear fuel. The researcher. define the continuously habitable zone of white dwarfs, and show that it extends from ~0,005 - 0,02 AU for white dwarfs with masses from 0,4 - 0,9 solar masses, temperatures less than 10,000 K, and habitable durations of at least 3 billion years. As they are similar in size to Earth, white dwarfs may be completely eclipsed by terrestrial planets that orbit edge-on, which can easily be detected with ground-based telescopes. If planets can migrate inward or reform near white dwarfs, The resaercher show that a global robotic telescope network could carry out a transit survey of nearby white dwarfs placing interesting constraints on the presence of habitable Earths. If planets were detected, He shows that the survey would favor detection of planets similar to Earth: similar size, temperature, rotation period, and host star temperatures similar to the Sun. The Large Synoptic Survey Telescope (LSST) could place even tighter constraints on the frequency of habitable Earths around white dwarfs. The confirmation and characterization of these planets might be carried out with large ground and space telescopes. Source: arXiv.org |




