Sentences with phrase «velocity method»

The phrase "velocity method" refers to a way of solving mathematical problems or analyzing data by looking at how quickly something is changing. It involves studying the speed at which something is moving or the rate at which something is happening. Full definition
«The most important discovery in this work is that we have detected the weakest signal and are reaching the limit of detecting Earth analogs using radial velocity method,» Feng said.
The failure, thus far, to find large substellar objects like brown dwarfs or a Jupiter - or Saturn - class planet in a «torch» orbit (closer than the Mercury to Sun distance) around 61 Ursae Majoris — with even the highly sensitive radial - velocity methods of Geoffrey W. Marcy and R. Paul Butler — bodes well for the possibility of Earth - type terrestrial planets around this star (Cumming et al, 1999).
I posed this same question to the person on stage in a 40 person presentation on Velocity method and the presenter gave some ridiculous response that didn't make any sense.
The planet was found with the radial velocity method, a planet - hunting technique that relies upon slight variations in the velocity of a star to determine the gravitational pull exerted by nearby planets that are too faint to observe directly with a telescope.
[4] Mass estimates for planets observed using the radial velocity method are lower estimates: if the planet's orbit is highly inclined it could have a higher mass and create the same observed effects.
This radial velocity method is extremely difficult for a planet with Earth's mass.
HARPS - North detects planets using the radial velocity method, which allows astronomers to measure a planet's mass.
The original claim was based on the radial velocity method — a planet - hunting technique which looks at how the gravitational pull of a planet slightly wobbles its star.
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.
The radial - velocity method has been an extraordinarily productive technique since it was used to identify the first exoplanet orbiting a sunlike star in 1995, but it yields a partial portrait of an exoplanet — revealing only lower bounds for planetary masses, for instance, which can produce ambiguities about whether a planet is rocky, like Earth, or gaseous, like Jupiter, or whether it is an even larger object such as a brown dwarf.
Additional simulation work presented in the paper also indicates that long - term telescopic observations may detect wobbles from such planets using the radial velocity method.
The new discoveries were made with the help of the radial velocity method, which looks for the periodic shifts of certain spectral lines in a star's light that are caused by the gravitational tug of invisible planets which orbit the star.
Using the ten - meter Keck I telescope fitted with the HIRES instrument, the team employed the radial velocity method to measure how much an orbiting planet causes its star to wobble, to determine the planet's mass.
Even though the radial velocity method can only give some rough measurements of an exoplanet's properties, like minimum mass and orbital period, it nevertheless allows astronomers to make some educated guesses regarding the planet's overall structure.
[94] Proxima Centauri b was found using the radial velocity method, where periodic Doppler shifts of spectral lines of the host star suggest an orbiting object.
Planet «b» or «1» - In 1996, a team of astronomers (including Geoffrey W. Marcy and R. Paul Butler) announced the discovery of a Jupiter - class planet around 47 UMa using highly sensitive radial - velocity methods (Fischer et al, 2001 — in pdf; and Butler and Marcy, 1996).
[109] The observational thresholds for planet detection in the habitable zones via the radial velocity method are currently (2017) estimated to be about 50 M ⊕ for Alpha Centauri A, 8 M ⊕ for B, and 0.5 M ⊕ for Proxima.
HD 211847's substellar companion, previously detected by the radial velocity method, is actually a low - mass star seen face - on.
In 1996, a team of astronomers (including Geoffrey W. Marcy and R. Paul Butler) announced the discovery of a Jupiter - class planet around 70 Virginis using highly sensitive radial - velocity methods (Marcy and Butler, 1996).
In 1996, a team of astronomers (including Eric Williams, Heather M. Hauser, and Phil Shirts) led by Geoffrey W. Marcy and R. Paul Butler announced the discovery of a Jupiter - class planet around Star A using highly sensitive radial - velocity methods (Butler et al, 1997).
(Many exoplanets have also been discovered using another technique called the radial velocity method, which looks for the gravitational influence of a planet on its star.)
By far the most successful technique for finding and studying extrasolar planets has been the radial velocity method, which measures the motion of host stars in response to gravitational tugs by their planets.
The failure, thus far, to find large substellar objects like brown dwarfs or a Jupiter - or Saturn - class planet in a «torch» orbit (closer than the Mercury to Sun distance) around Xi Boötis A — with even the highly sensitive radial - velocity methods of Geoffrey W. Marcy and R. Paul Butler — bodes well for the possibility of Earth - type terrestrial planets around this star (Cumming et al, 1999).
Most importantly, as Feng explained via an email exchange shared with Gizmodo, the research pushes the limits of the sorts of planets we can detect with the radial velocity method, boosting our prospects of discovering truly Earth - sized, rocky worlds in the future.
The transit method, the radial velocity method, and the transit timing variation method are also indirect detection methods.
HARPS has been enormously successful at detecting exoplanets using the radial velocity method, or measuring the gravitational tugs on stars by their planets by watching the stars» spectral lines «wobble» back and forth due to the Doppler effect.
Neither the transit method nor the radial velocity method are able to detect such a small planet so far away, which shows how incredible microlensing planets can be.
Significantly, the researchers say they have improved the precision of the radial velocity method to arrive at these revised estimates.
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.

Phrases with «velocity method»

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