|
|
發表於 2013-1-26 15:46:45
|
顯示全部樓層
An extrasolar planet
[youtubeHD=640,420]d0c1_gjChYw[/youtubeHD]
An extrasolar planet, or exoplanet, is a planet outside the Solar System. A total of 859 such planets (in 676 planetary systems, including 128 multiple planetary systems) have been identified as of January 23, 2013. The Kepler mission has detected over 18,000 additional candidates, including potentially 262 habitable ones. In the Milky Way galaxy, it is expected that there are many billions of planets (at least one planet per star, resulting in 100-400 billion exoplanets) not only occurring around the stars but also as free-floating planetary-mass bodies. The nearest known exoplanet is Alpha Centauri Bb. Almost all of the planets detected so far are within our home galaxy the Milky Way; however, there have been a small number of possible detections of extragalactic planets. Astronomers at the Harvard-Smithsonian Center for Astrophysics (CfA) reported in January 2013, that "at least 17 billion" Earth-sized exoplanets are estimated to reside in the Milky Way Galaxy.
For centuries, many philosophers and scientists supposed that extrasolar planets existed, but there was no way of knowing how common they were or how similar they might be to the planets of the Solar System. Various detection claims, starting in the nineteenth century, were all eventually rejected by astronomers. The first confirmed detection came in 1992, with the discovery of several terrestrial-mass planets orbiting the pulsar PSR B1257+12. The first confirmed detection of an exoplanet orbiting a main-sequence star was made in 1995, when a giant planet was found in a four-day orbit around the nearby star 51 Pegasi. Due to improved observational techniques, the rate of detections has increased rapidly since then. Some exoplanets have been directly imaged by telescopes, but the vast majority have been detected through indirect methods such as radial velocity measurements.Besides exoplanets, "exocomets", comets beyond our solar system, have also been detected and may be common in the Milky Way Galaxy.
Infrared observations of infrared observations of extrasolar planets extrasolar planets
[youtubeHD=640,420]KUZyn5PhRJg[/youtubeHD]
Most known exoplanets are giant planets believed to resemble Jupiter or Neptune, but this reflects a sampling bias, as massive planets are more easily observed. Some relatively lightweight exoplanets, only a few times more massive than Earth (now known by the term Super-Earth), are known as well; statistical studies now indicate that they actually outnumber giant planets while recent discoveries have included Earth-sized and smaller planets and a handful that appear to exhibit other Earth-like properties.There also exist planetary-mass objects that orbit brown dwarfs and other bodies that "float free" in space not bound to any star; however, the term "planet" is not always applied to these objects.
The discovery of extrasolar planets, particularly those that orbit in the habitable zone where it is possible for liquid water to exist on the surface (and therefore also life), has intensified interest in the search for extraterrestrial life. Thus, the search for extrasolar planets also includes the study of planetary habitability, which considers a wide range of factors in determining an extrasolar planet's suitability for hosting life.
On January 7, 2013, astronomers from the Kepler Mission space observatory announced the discovery of KOI-172.02, an Earth-like exoplanet candidate orbiting a star similar to our Sun in the habitable zone and possibly a "prime candidate to host alien life".
|
|
樓主: 趙雲[子龍]
在線雷達
發表於 2013-1-26 17:32:45
