Radial
velocity measurements determine the sizes and shapes of the orbits of extrasolar planets as well as the lower limits of the masses of these planets.
Not exact matches
It appears to be a main sequence red dwarf star of spectral and luminosity type M4.5 V. Because of its small mass and great distance from the primary (Star A), Upsilon Andromedae B appears to have a negligible effect on the radial
velocity measurements used to
determine that Star A has at least three large planets (Lowrance et al, 2002).
So
velocity measurements help to group objects together but do not
determine the distances for those groups.
Older calculations indicating that the Wolf 424 system would get as close to the Solar System as 0.95 light - years within around 7,500 years have been
determined to be based on a «probably erroneous» radial
velocity measurement (Vadim V. Bobylev, 2010; and Mülläri and Orlov, 1996).
Furthermore, by knowing the mass of a planet from radial
velocity measurements and the radius of a planet based on how much starlight it blocked, it is a simple calculation to
determine a planet's density, which can tell astronomers whether that planet is rocky or gaseous in nature, or whether it has a small core and a thick atmosphere, or whether it has a large core covered in deep oceans.
Putting the
measurements together, the team
determined the star is moving at about 1,200 kilometers per second — much higher than the
velocities of previously known stars in the Milky Way galaxy.
By re-observing the photometric transit, we attempt to
determine the transit parameters to high precision, and, by spectroscopic observations, to estimate the properties of the host star and
determine the mass of the transiting object by means of radial -
velocity measurements.
Using this tool, we can
determine heart function based on dynamic
measurements (contraction of the heart, chamber size and blood
velocity).
I can
determine the standard uncertainty for all the measured variables from statistics It is falsifiable — i can move a body at a certain
velocity for a certain time and measure the traveled distance If the traveled distance does not fit with calculated distance within the uncertainty calculated by using the international standard Guide to the expression of Uncertainty in
Measurement the model might be wrong.
To
determine how much ice and snowfall enters a specific ice shelf and how much makes it to an iceberg, where it may split off, the research team used a regional climate model for snow accumulation and combined the results with ice
velocity data from satellites, ice shelf thickness
measurements from NASA's Operation IceBridge — a continuing aerial survey of Earth's poles — and a new map of Antarctica's bedrock.