Sentences with phrase «distance to the star»

This technique, called parallax, has measured distances to stars since the 1830s.

Astronomers use a technique called parallax to precisely measure to distance to stars in the sky.

The VLBA measurements, made in the spring and fall, allow the team to calculate distances to the stars and construct a map of the galaxy.

Walking distance to the Star Market that sells booze, one of the few grocery stores that sell alcohol in this this state!

Together with observations from more northern latitudes, Cook's 1769 data provided the first accurate distance to our star — and by extension, to the rest of the planets in the solar system.

Image of HD 115600 showing a bright debris ring viewed nearly edge - on and located just beyond a Pluto - like distance to the star.

One of the biggest obstacles to getting better precision, says Riess, is measuring distances to stars within the Milky Way that he and his colleagues can use to calibrate the brightness of type 1a supernovas.

Stellar Parallax measures the distance to stars based on the mathematical knowlege of the geometry of earth's orbit around the sun.

Leavitt worked out the «period - luminosity relationship» in 1908, giving astronomers a powerful tool for measuring the distance to stars and other astronomical objects.

The astronomers used a technique called trigonometric parallax, first used in 1838 to measure the distance to a star.

Astronomers using the National Science Foundation's Very Long Baseline Array (VLBA) have directly measured the distance to a star - forming region on the opposite side of our Milky Way Galaxy from the Sun.

Comparing this with the apparent brightness yields the distance to the star and galaxy.

The researchers identified about 1650 such stars and then estimated the distance to those stars (red dots in image; the black dot denotes the position of our solar system).

Their observations and ideas, described in a new book, led to such advances in astronomy as how to measure the distance to stars.

If you know the distance to a star, you can determine its luminosity and mass.

Other factors that broaden the main sequence band on the HR diagram include uncertainty in the distance to stars and the presence of unresolved binary stars that can alter the observed stellar parameters.

The data collected by Spitzer and other telescopes reveal the exoplanets» sizes and distances to their stars, while theoretical models predict additional information about the planets» atmospheres and surfaces.

It turns out that measuring the distance to a star is an interesting problem!

If they know the star's brightness and the distance to the star, they can calculate its luminosity — the amount of energy that it puts out (luminosity = brightness x 12.57 - x (distance) 2 --RRB-.

The brightness of a star is inversely proportional to the square of the distance to that star.

But the Pale Red Dot campaign, an initiative that is searching for planets orbiting Proxima Centauri, was only able to determine Proxima b's orbit and the distance to its star, based on wobbles that the planet's motion induces in the star.

If they know the star's brightness and the distance to the star, they can calculate the star's luminosity:

Students use the parallax formula to calculate the distances to stars in Orion.