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.
Not exact matches
Data
from amateurs is important because professionals do not have the time or money to observe every
planetary transit at major observatories.
This was borne out by his first voyage in 1768 on the Endeavour with James Cook, who was to observe the
transit of Venus across the face of the Sun
from the southern hemisphere to help to calculate
planetary distances, while Banks collected biological specimens, the first
from the South Pacific to be seen in England.
They plan to test - drive the telescope's instruments on two
transiting Jupiter - size worlds, WASP - 39 b and WASP - 43 b, gleaning as much data as possible
from the shifting patterns of starlight and
planetary shadow.
KELT - 6b is now the longest - duration full
planetary transit continuously observed
from the ground, she said.
It was looking for
planetary «
transits,» in which fortuitously aligned worlds cross the face of their host stars and block a fraction of the starlight seen
from Earth.
The few known super-Earths whose orbits are fortuitously aligned so that they
transit — pass in front of their host star —
from Earth's vantage point provide a unique laboratory for
planetary investigations.
It spends much of its time monitoring the light
from around 60 of the nearest ultracool dwarf stars and brown dwarfs («stars» which are not quite massive enough to initiate sustained nuclear fusion in their cores), looking for evidence of
planetary transits.
Coming hot off the heels of discoveries made by other observatories, including NASA's Kepler and CoRot (the Convection, Rotation, and
Planetary Transits mission, led by France's CNES with contributions
from the ESA), this spacecraft is intended to build significantly on our knowledge of the universe, the Solar System, and the formation of life in general.
From the European Space Agency (ESA): «The
PLAnetary Transits and Oscillations of stars (PLATO) mission will identify and study thousands of exoplanetary systems, with an emphasis on discovering and characterising Earth - sized planets and super-Earths.
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.
The expected Doppler signals are too small to confirm them by demonstrating that their masses are in the
planetary regi... ▽ More We present an investigation of twelve candidate
transiting planets
from Kepler with orbital periods ranging
from 34 to 207 days, selected
from initial indications that they are small and potentially in the habitable zone (HZ) of their parent stars.
The first, shows the difference between the actual length of day and 86,400 SI seconds (24 hours) over the past two and a half thousand years estimated
from records of various astronomical events (eclipses,
planetary transits, occultations etc).
For Kepler - 20c and Kepler - 20d, the blend scenario is independently disfavored by the achromaticity of the
transit:
From Spitzer data gathered at 4.5 um, we infer a ratio of the
planetary to stellar radii of 0.075 + -0.015 (Kepler - 20c) and 0.065 + -0.011 (Kepler - 20d), consistent with each of the depths measured in the Kepler optical bandpass.
We combine the estimate of Teff and [Fe / H] with an estimate o... ▽ More We present the discovery of the Kepler - 19
planetary system, which we first identified
from a 9.3 - day periodic
transit signal in the Kepler photometry.
Abstract: We present the discovery of the Kepler - 19
planetary system, which we first identified
from a 9.3 - day periodic
transit signal in the Kepler photometry.
We apply a statistical method to show that the likelihood of the
planetary interpretation of the
transit signals is more than three orders of magnitude larger than that of the alternative hypothesis that the signals result
from an eclipsing binary star.
Solutions for stellar parallax and proper motions await more observations, but the analysis of the astrometric residuals
from a local solution in the vicinity of a star have already proved to be an important tool in the process of confirming the hypothesis of a
planetary transit.
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.
The 16
planetary candidates have estimated diameters within range of being super-Earths (1.26 to 2.0 times Earth's diameter), given error margins ranging
from 25 to 35 percent due to the uncertainty in the size of their host star and of the «depth» of the observed
transits (decrease in stellar luminosity) across the surface of the star.
We report on the results
from the radial - velocity follow - up program performed to establish the
planetary nature and to characterize the
transiting candidates discovered by the space mission CoRoT.
At EVE Fanfest 2017, it was announced that that players of MMO EVE Online will soon be joining the great exoplanet hunt too through an interesting new mini-game that challenges players to find elusive
planetary transits in data
from telescopes around the world.