That is why
the first radial velocity planet (51 Peg), the first transiting planet (OGLE - TR - 056), the first microlensing planet (OGLE 2003 - BLG - 235L), and the first directly imaged planet (GQ Lupi b) were all Jupiter - like or larger.
We believe this was
the first radial velocity detection of an extrasolar planet by amateurs.
Not exact matches
The planet was found using the
radial velocity method: Telescopes scrutinize a star's light to see if its frequency is periodically stretched and squeezed by the Doppler effect as the star is tugged,
first away and then toward us, by an orbiting planet.
I. Performances of
radial velocity measurements,
first analyses of variations.
Abstract: Kepler - 10b was the
first rocky planet detected by the Kepler satellite and con - firmed with
radial velocity follow - up observations from Keck - HIRES.
When we
first embarked on this project we were told unequivocally that precision
radial velocity measurements were impossible at the amateur level and required the funding and resources of an institution.
When the
first exoplanet was identified via the
radial velocity method, the Swiss team was able to detect a wobble in the star 51 Pegasi at a rate of 50 meters per second.
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.