'Extrasolar' web sites
The extrasolar planet encyclopaedia mdash; tau cet b
exoplanet.eu 2015-08-13 ⚑news
extrasolar Planet Encyclopaedia mdash; tau Cet b Home All Catalogs Diagrams Bibliography Research Meetings Other Sites VO Planet tau Cet b Name tau Cet b Discovered in 2012 Mass 0.0063 0.0025 MJ Semi.major axis 0.105 0.006 AU Orbital period 13.965 0.02 day Eccentricity 0.16.0.22 0.16 85.5 deg Tperi 2450004.17 JD Radius mdash; Inclination mdash; Update May 5, 2015 Detection Method Controversial Mass Detection Method mdash; Radius
exoplanet.eu 2015-08-13 ⚑news
extrasolar Planet Encyclopaedia mdash; tau Cet b Home All Catalogs Diagrams Bibliography Research Meetings Other Sites VO Planet tau Cet b Name tau Cet b Discovered in 2012 Mass 0.0063 0.0025 MJ Semi.major axis 0.105 0.006 AU Orbital period 13.965 0.02 day Eccentricity 0.16.0.22 0.16 85.5 deg Tperi 2450004.17 JD Radius mdash; Inclination mdash; Update May 5, 2015 Detection Method Controversial Mass Detection Method mdash; Radius
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The extrasolar planet encyclopaedia mdash; tau cet c
extrasolar Planet Encyclopaedia mdash; tau Cet c Home All Catalogs Diagrams Bibliography Research Meetings Other Sites VO Planet tau Cet c Name tau Cet c Discovered in 2012 Mass 0.0098 0.0044 MJ Semi.major axis 0.195 0.01 AU Orbital period 35.362 0.1 day Eccentricity 0.03.0.3 0.03 170.0 deg Tperi 2450020.62 JD Radius mdash; Inclination mdash; Update May 5, 2015 Detection Method Controversial Mass Detection Method mdash; Radius
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The extrasolar planet encyclopaedia mdash; tau cet d
extrasolar Planet Encyclopaedia mdash; tau Cet d Home All Catalogs Diagrams Bibliography Research Meetings Other Sites VO Planet tau Cet d Name tau Cet d Discovered in 2012 Mass 0.011 0.005 MJ Semi.major axis 0.374 0.02 AU Orbital period 94.11 0.7 day Eccentricity 0.08.0.26 0.08 228.0 deg Tperi 245002.31 JD Radius mdash; Inclination mdash; Update May 5, 2015 Detection Method Controversial Mass Detection Method mdash; Radius
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Www.wasp.le.ac.uk. the superwasp public archive
www.wasp.le.ac.uk 2012-02-07
extrasolar planet project based in the UK. It works by imaging large parts of the sky and creating light curves of every star to search for characteristics of an exo.planet transit. This means there are literally millions of light curves that contain interesting non extrasolar planet science that have never been looked at. To find out more about how the project works have a look at the main project webpage. Examples of the non
www.wasp.le.ac.uk 2012-02-07
extrasolar planet project based in the UK. It works by imaging large parts of the sky and creating light curves of every star to search for characteristics of an exo.planet transit. This means there are literally millions of light curves that contain interesting non extrasolar planet science that have never been looked at. To find out more about how the project works have a look at the main project webpage. Examples of the non
Transitsearch. news
www.oklo.org 2015-08-13 ⚑news
extrasolar Search Team published on astro.ph yesterday announces the discovery of highly eccentric planets orbiting the sunlike stars HD 156846 and HD 4113. The newly discovered planets have orbital periods of 359.5 and 526.6 days, and eccentricities, e 0.847 and e 0.903, respectively. Normally, planets with such long periods make poor Transitsearch.org candidates, due low a.priori transit probabilities and highly uncertain
www.oklo.org 2015-08-13 ⚑news
extrasolar Search Team published on astro.ph yesterday announces the discovery of highly eccentric planets orbiting the sunlike stars HD 156846 and HD 4113. The newly discovered planets have orbital periods of 359.5 and 526.6 days, and eccentricities, e 0.847 and e 0.903, respectively. Normally, planets with such long periods make poor Transitsearch.org candidates, due low a.priori transit probabilities and highly uncertain
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Transitsearch. getting started
extrasolar planets, and was a member of the XO network, which has had made several discoveries of new transiting planets. Bruce has written a book, Exoplanet Observing for Amateurs which he made available for free in.pdf form. copyright 2000.2009. All Rights
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Systemic console tutorial 4
systemic Console Tutorial 4 systemic characterizing planetary systems Home About Downloadable Console Console Tutorial 1 Console Tutorial 2 Console Tutorial 3 Console Tutorial 4 Console Tutorial 4 February 23rd, 2011 Leave a comment Go to comments 61 Vir 61 Virginis shown above in a Goddard SkyView image is one of only a handful of truly Sun.like stars that can be seen with the naked eye. It lies in the constellation Virgo, with a
Mt. hamilton telescopes carnegie double astrograph
www.ucolick.org 2013-03-21 ⚑r&d
extrasolar planetary research has been very successful at Lick Observatory, yet observing time on the Shane telescope for any one project is extremely limited. By operating robotically every on clear night, APF will greatly increase chances of detecting extrasolar planets. APF more efficient system and higher resolution spectrometer will increase astronomers ability to detect these planets. APF consists of a 2.4.meter automated
www.ucolick.org 2013-03-21 ⚑r&d
extrasolar planetary research has been very successful at Lick Observatory, yet observing time on the Shane telescope for any one project is extremely limited. By operating robotically every on clear night, APF will greatly increase chances of detecting extrasolar planets. APF more efficient system and higher resolution spectrometer will increase astronomers ability to detect these planets. APF consists of a 2.4.meter automated
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Professor steven s. vogt
extrasolar planetary system with three potentially habitable planets. GJ 667C, a nearby low.mass star, is the first star to known host several Super.earth planets in its habitable zone. In this planetary system, the habitable zone lies entirely within an orbit the size of Mercury, much closer in than for our Sun. The findings are based in part on data that Paul Butler and I have taken over the past 13 years using the HIRES
California planet search
exoplanets.org 2016-01-10
extrasolar Planet News Planetary Systems Displayed PREVIOUS DISCOVERIES.June 13, 2005. A 7.5 Earth.mass planet..Sept. 1, 2004. The First Two Neptune.Class Exoplanets.. September 17, 2002. Another Jupiter.sized planet in a circular orbit.. June 13, 2002. 15 New Planets; 3 New Multiple.Planet Systems; Smallest Exoplanet yet discovered.. February 7, 2002. A New Planet 12 Times Jupiter Mass.. January 8, 2002. Planet Orbiting a Giant
exoplanets.org 2016-01-10
extrasolar Planet News Planetary Systems Displayed PREVIOUS DISCOVERIES.June 13, 2005. A 7.5 Earth.mass planet..Sept. 1, 2004. The First Two Neptune.Class Exoplanets.. September 17, 2002. Another Jupiter.sized planet in a circular orbit.. June 13, 2002. 15 New Planets; 3 New Multiple.Planet Systems; Smallest Exoplanet yet discovered.. February 7, 2002. A New Planet 12 Times Jupiter Mass.. January 8, 2002. Planet Orbiting a Giant
H2g2. categories
www.h2g2.com 2014-11-14
extrasolar Planets 8 Families 66 Food DrinkGeneral Astronomy 83 Health Healing 1 History PoliticsHolidays Observances 51 Human Behaviour 5 Languages LinguisticsLaw Crime 83 Leisure LifestyleMaths, Science Technology Mythology FolkloreSexSociety and Cultures 114 Space, Stars and Galaxies 76 SportsThe EarthThe Natural WorldThe Solar System 23 Travel TransportWork See Also All About h2g2 4 The UnderGuide 5 The World of h2g2 4 The
www.h2g2.com 2014-11-14
extrasolar Planets 8 Families 66 Food DrinkGeneral Astronomy 83 Health Healing 1 History PoliticsHolidays Observances 51 Human Behaviour 5 Languages LinguisticsLaw Crime 83 Leisure LifestyleMaths, Science Technology Mythology FolkloreSexSociety and Cultures 114 Space, Stars and Galaxies 76 SportsThe EarthThe Natural WorldThe Solar System 23 Travel TransportWork See Also All About h2g2 4 The UnderGuide 5 The World of h2g2 4 The
Hubble confirms young planet at nearby star. space.com
space.com 2012-11-19 ⚑xxx
extrasolar planets found to date orbit incredibly close to their host stars. In some systems, Jupiter.sized worlds orbit a star in just a few days. Other planets take wildly eccentric paths around their stars. The findings are detailed in the June 23 issue of the journal Nature. Early Earth Not So Hellish, New Study Suggests 10 Years of Planet Hunting Amazing Variety Out There Eccentric Worlds Strange Orbits Puzzle Astronomers
space.com 2012-11-19 ⚑xxx
extrasolar planets found to date orbit incredibly close to their host stars. In some systems, Jupiter.sized worlds orbit a star in just a few days. Other planets take wildly eccentric paths around their stars. The findings are detailed in the June 23 issue of the journal Nature. Early Earth Not So Hellish, New Study Suggests 10 Years of Planet Hunting Amazing Variety Out There Eccentric Worlds Strange Orbits Puzzle Astronomers
Cnn.com. earth moon could become a planet. aug 18, 2006
edition.cnn.com 2012-07-21 ⚑finance ⚑video
extrasolar planet researcher at the University of California, Santa Cruz.The new definition, proposed this week by the International Astronomical Union IAU , basically says every round object orbiting the sun is a planet, unless it orbits another planet. But there is a big caveat If the center of gravity, called the barycenter, is outside the larger object, then the smaller object is a planet. That wording elevates Pluto moon
edition.cnn.com 2012-07-21 ⚑finance ⚑video
extrasolar planet researcher at the University of California, Santa Cruz.The new definition, proposed this week by the International Astronomical Union IAU , basically says every round object orbiting the sun is a planet, unless it orbits another planet. But there is a big caveat If the center of gravity, called the barycenter, is outside the larger object, then the smaller object is a planet. That wording elevates Pluto moon
The eventful universe. schedule
www.noao.edu 2012-02-21
extrasolar Planet Tracker Instruments Jian Ge V. Really Interesting Ways to Find Interesting Stuff 11 15 Transient Identification and Classification with WISE Douglas Hoffman 11 30 WISE Clear Views of Dark Objects Roc Cutri 11 45 Reaching Out with Eventful Astronomy Kirk Borne 12 00 Lunch on your own 01 30 SOFIA and Astronomical Transient Events Dan Lester 01 45 Search for Hidden Baryons Through Scintillation Marc Moniez 02 00 The
www.noao.edu 2012-02-21
extrasolar Planet Tracker Instruments Jian Ge V. Really Interesting Ways to Find Interesting Stuff 11 15 Transient Identification and Classification with WISE Douglas Hoffman 11 30 WISE Clear Views of Dark Objects Roc Cutri 11 45 Reaching Out with Eventful Astronomy Kirk Borne 12 00 Lunch on your own 01 30 SOFIA and Astronomical Transient Events Dan Lester 01 45 Search for Hidden Baryons Through Scintillation Marc Moniez 02 00 The
Space dew. the search engine dedicated to astronomy and space
www.spacedew.com 2006-11-20
extrasolar Planets Famous Scientists History Libraries Chemistry. Engineering. Mathematics. Physics and Astronomy Light Pollution Magazines and eZines Newsletters Observatories Cosmic. Optical. Radio. Solar. Space Physics Physicists. Quantum. Relativity Picture Images Planetariums around the world Planets Mars Software Solar System Space Agencies NASA Space for Kids Space Camp Space News Online Space Satellites and Programs Space
www.spacedew.com 2006-11-20
extrasolar Planets Famous Scientists History Libraries Chemistry. Engineering. Mathematics. Physics and Astronomy Light Pollution Magazines and eZines Newsletters Observatories Cosmic. Optical. Radio. Solar. Space Physics Physicists. Quantum. Relativity Picture Images Planetariums around the world Planets Mars Software Solar System Space Agencies NASA Space for Kids Space Camp Space News Online Space Satellites and Programs Space
The extrasolar planet encyclopaedia mdash; tau cet b
exoplanet.eu 2015-08-13 ⚑news
extrasolar Planet Encyclopaedia mdash; tau Cet b Home All Catalogs Diagrams Bibliography Research Meetings Other Sites VO Planet tau Cet b Name tau Cet b Discovered in 2012 Mass 0.0063 0.0025 MJ Semi.major axis 0.105 0.006 AU Orbital period 13.965 0.02 day Eccentricity 0.16.0.22 0.16 85.5 deg Tperi 2450004.17 JD Radius mdash; Inclination mdash; Update May 5, 2015 Detection Method Controversial Mass Detection Method mdash; Radius
exoplanet.eu 2015-08-13 ⚑news
extrasolar Planet Encyclopaedia mdash; tau Cet b Home All Catalogs Diagrams Bibliography Research Meetings Other Sites VO Planet tau Cet b Name tau Cet b Discovered in 2012 Mass 0.0063 0.0025 MJ Semi.major axis 0.105 0.006 AU Orbital period 13.965 0.02 day Eccentricity 0.16.0.22 0.16 85.5 deg Tperi 2450004.17 JD Radius mdash; Inclination mdash; Update May 5, 2015 Detection Method Controversial Mass Detection Method mdash; Radius
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The extrasolar planet encyclopaedia mdash; tau cet c
extrasolar Planet Encyclopaedia mdash; tau Cet c Home All Catalogs Diagrams Bibliography Research Meetings Other Sites VO Planet tau Cet c Name tau Cet c Discovered in 2012 Mass 0.0098 0.0044 MJ Semi.major axis 0.195 0.01 AU Orbital period 35.362 0.1 day Eccentricity 0.03.0.3 0.03 170.0 deg Tperi 2450020.62 JD Radius mdash; Inclination mdash; Update May 5, 2015 Detection Method Controversial Mass Detection Method mdash; Radius
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The extrasolar planet encyclopaedia mdash; tau cet d
extrasolar Planet Encyclopaedia mdash; tau Cet d Home All Catalogs Diagrams Bibliography Research Meetings Other Sites VO Planet tau Cet d Name tau Cet d Discovered in 2012 Mass 0.011 0.005 MJ Semi.major axis 0.374 0.02 AU Orbital period 94.11 0.7 day Eccentricity 0.08.0.26 0.08 228.0 deg Tperi 245002.31 JD Radius mdash; Inclination mdash; Update May 5, 2015 Detection Method Controversial Mass Detection Method mdash; Radius
Transitsearch. news
www.oklo.org 2015-08-13 ⚑news
extrasolar Search Team published on astro.ph yesterday announces the discovery of highly eccentric planets orbiting the sunlike stars HD 156846 and HD 4113. The newly discovered planets have orbital periods of 359.5 and 526.6 days, and eccentricities, e 0.847 and e 0.903, respectively. Normally, planets with such long periods make poor Transitsearch.org candidates, due low a.priori transit probabilities and highly uncertain
www.oklo.org 2015-08-13 ⚑news
extrasolar Search Team published on astro.ph yesterday announces the discovery of highly eccentric planets orbiting the sunlike stars HD 156846 and HD 4113. The newly discovered planets have orbital periods of 359.5 and 526.6 days, and eccentricities, e 0.847 and e 0.903, respectively. Normally, planets with such long periods make poor Transitsearch.org candidates, due low a.priori transit probabilities and highly uncertain
MORE
ⓘ
Systemic console tutorial 4
systemic Console Tutorial 4 systemic characterizing planetary systems Home About Downloadable Console Console Tutorial 1 Console Tutorial 2 Console Tutorial 3 Console Tutorial 4 Console Tutorial 4 February 23rd, 2011 Leave a comment Go to comments 61 Vir 61 Virginis shown above in a Goddard SkyView image is one of only a handful of truly Sun.like stars that can be seen with the naked eye. It lies in the constellation Virgo, with a
Hubble confirms young planet at nearby star. space.com
space.com 2012-11-19 ⚑xxx
extrasolar planets found to date orbit incredibly close to their host stars. In some systems, Jupiter.sized worlds orbit a star in just a few days. Other planets take wildly eccentric paths around their stars. The findings are detailed in the June 23 issue of the journal Nature. Early Earth Not So Hellish, New Study Suggests 10 Years of Planet Hunting Amazing Variety Out There Eccentric Worlds Strange Orbits Puzzle Astronomers
space.com 2012-11-19 ⚑xxx
extrasolar planets found to date orbit incredibly close to their host stars. In some systems, Jupiter.sized worlds orbit a star in just a few days. Other planets take wildly eccentric paths around their stars. The findings are detailed in the June 23 issue of the journal Nature. Early Earth Not So Hellish, New Study Suggests 10 Years of Planet Hunting Amazing Variety Out There Eccentric Worlds Strange Orbits Puzzle Astronomers
Cnn.com. earth moon could become a planet. aug 18, 2006
edition.cnn.com 2012-07-21 ⚑finance ⚑video
extrasolar planet researcher at the University of California, Santa Cruz.The new definition, proposed this week by the International Astronomical Union IAU , basically says every round object orbiting the sun is a planet, unless it orbits another planet. But there is a big caveat If the center of gravity, called the barycenter, is outside the larger object, then the smaller object is a planet. That wording elevates Pluto moon
edition.cnn.com 2012-07-21 ⚑finance ⚑video
extrasolar planet researcher at the University of California, Santa Cruz.The new definition, proposed this week by the International Astronomical Union IAU , basically says every round object orbiting the sun is a planet, unless it orbits another planet. But there is a big caveat If the center of gravity, called the barycenter, is outside the larger object, then the smaller object is a planet. That wording elevates Pluto moon
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