Examples of using The parallax in English and their translations into Vietnamese
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It is sufficiently near that the distance can be measured directly using the parallax technique and such measurements obtained during the Hipparcos mission yield an estimate of approximately 300 light-years(90 parsecs) from the Sun.[2].
while Cassini stayed in Paris so that the two could make simultaneous observations of Mars and, by computing the parallax, determined its distance from Earth.
One of the reasons one page websites are so attractive is because they make great use of the parallax effect to add visual appeal without slowing your website down.
star(61 Cygni at 11.4 light-years) was made in 1838 by Friedrich Bessel using the parallax technique.
In practice, however, the method cannot be applied, because the Sun's intense glare blots out the background stars needed for the parallax measurement.
In 1672 the Italian-born French astronomer Gian Domenico Cassini made a reasonably close estimate of the astronomical unit based on a determination of the parallax displacement of the planet Mars- and thus its distance to Earth.
In 1882-3, the parallax of ε Indi was measured by astronomers David Gill and William L. Elkin
and calculating the parallax of the sun.
would have been 18.5) and high uncertainty in the parallax suggested that it was in fact somewhat farther away,
The parallax angle is found by measuring the parallax motion(or apparent movement of a star relative to stable, more distant stars) when the star is
However, the Aristotelian viewpoint proved more influential, and it was not until the 16th century that Tycho Brahe demonstrated that comets must exist outside the Earth's atmosphere by measuring the parallax of the Great Comet of 1577 from observations collected by geographically separated observers.
Claude-Louis Mathieu in 1812, who recorded the parallax at 500 milliarcseconds(mas),
1900-1901 allowed a considerable improvement in parallax measurement.[45] Another international project to measure the parallax of 433 Eros was undertaken in 1930-1931.[38][46].
For terrestrial observations,"Sun- object- Earth" is often nearly the same thing as"Sun- object- observer", since the difference depends on the parallax, which in the case of observations of the Moon can be as much as 1°, or two full Moon diameters.
Adjusting the Parallax.
Parallax backgrounds- Like the parallax effect?
The parallax was initially measured as 0.43± 0.13 arcseconds.
He then decides to enroll for the Parallax training himself to discover the truth.
Measuring the parallax of stars in our galaxy, including some Cepheids.