Bean tracked GJ 1214 b through two of
those planetary transits using one of the 8.2 - meter telescopes at the Very Large Telescope atop Cerro Paranal in Chile, parsing the observed light into its individual wavelengths.
Not exact matches
To confirm that the
transits of COROT 9 b recorded in 2008 by the COROT satellite were indeed
planetary, the researchers first took two follow - up readings of the star
using a spectrograph in France, a rough sketch that was consistent with the presence of a planet.
All of the potentially Earth - like worlds were spotted
using the
transit method, which measures dips in a star's light output as a
planetary body crosses in front from our line of sight.
This observational result, which
uses the achromatic property of
planetary transit signals that is not investigated by the Kepler observations, provides an independent indication that Kepler's false positive rate is low.
The initial
transit signal was identified in KELT - North survey data, and the
planetary nature of the occulter was established
using a combination of follow - up photometry, high - resolution imaging, high - resolution spectroscopy, and precise radial velocity measurements.
We confirmed the
planetary nature of the
transiting companion
using this mass limit and Doppler tomographic observations to verify that the companion
transits HD 332124.
We confirmed the
planetary nature of the
transiting companion
using this mass limit and Doppler tom... ▽ More We present the discovery of KELT - 21b, a hot Jupiter
transiting the $ V = 10.5 $ A8V star HD 332124.
Using the very high precision Kepler photometry, and follow - up observations, our confidence that these signals represent
planetary transits is > 99.1 %.
Forty precision Doppler measurements were
used to confirm that the short - period
transit event is due to a
planetary companion.
A third mission, called PLATO (
PLAnetary Transits and Oscillations of stars), proposed
using a number of small, optically fast, wide - field telescopes to detect and characterize a large number of close - by exoplanetary systems.
On December 16, 2009, a team of astronomers (including David Charbonneau, Zachory K. Berta, Jonathan Irwin, Christopher J. Burke, Philip Nutzman, Lars A. Buchhave, Christophe Lovis, Xavier Bonfils, David W. Latham, Stéphane Udry, Ruth A. Murray - Clay, Matthew J. Holman, Emilio E. Falco, Joshua N. Winn, Didier Queloz, Francesco Pepe, Michel Mayor, Xavier Delfosse, and Thierry Forveille) announced the discovery of a planet «b» of 6.55 ± 0.98 Earth - masses in a tight inner orbit
using the «
transit method» of
planetary detection
using «a fleet of ground - based telescopes no larger than those many amateur astronomers have in their backyards» as part of the MEarth Project (CfA news release).
On December 16, 2009, a team of astronomers announced the discovery of a super-Earth in an inner orbit
using the «
transit method» of
planetary detection
using «a fleet of ground - based telescopes no larger than those many amateur astronomers have in their backyards» as part of the MEarth Project (CfA news release).
On Wednesday, February 2, 2011, NASA's Kepler Mission revealed that, thus far, it has detected 1,235
planetary candidates orbiting 907 host stars, from a survey of some 155,453 stars in constellations Cygnus and Lyra
using the
transit method which requires a rare orbital alignment across the face of the host star as seen from the Solar System.
He is one of the discovers of the first ring around an asteroid (Chariklo) and with collaborators was the one to first
use measurements of
planetary transits from space to measure the size of the sun.
We first generate a stellar field with
planetary companions based on radial velocity discoveries,
use a
planetary evolution model assuming a variable fraction of heavy elements to compute the characteristics of
transit events, then apply a detection criterion that includes both statistical and red noise sources.