In kilometres, including the dwarf planet Pluto:
Mercury: 57,910,000
Venus: 108,200,000
Earth: 149,600,000
Mars: 227,940,000
Jupiter: 778,330,000
Saturn: 1,426,980,000
Uranus: 2,870,990,000
Neptune: 4,497,070,000
Pluto: 5,913,520,000
In miles:
Mercury: 35,985,274
Venus: 67,235,480
Earth: 92,961,440
Mars: 141,641,916
Jupiter: 483,654,262
Saturn: 886,725,372
Uranus: 1,784,033,186
Neptune: 2,794,479,298
Pluto: 3,674,661,328
It depends on the distance they are measuring. For things very very close in space they use kilometers. For things a bit farther away, like planets, they use Astronomical units (au). For things way out there, like stars, they use light-years.
The formula you use to find that distance depends on whether the planet is closer to the sun than Earth (Inferior) or further than Earth (superior)
http://astro.unl.edu/naap/ssm/ssm_advanced.html
that website derives the formulas for you as well as giving you the formula to plug your numbers into.
Parallax, measured in parsecs. One parsec is the distance where the star seems to move one parallax second of arc when measured against the far more distant background stars. It is just over 3 light years.
Stars.
The Parallax Method. See the link for more info.
For nearby stars, the parallax method is used.
Not if they have the faintest clue what they're doing. Parallax is used to measure distance, not temperature.
In 1838 Friedrich Bessel was able to measure the parallax of the nearby star 61 Cygni and thus determine its distance and independenly confirm the fact that the Earth orbits round the Sun.
To measure the distance from the earth to the sun, or to any star for that matter astronomers use a form of trigonometry called Parallax (see related Link). Simply put, think of measuring a known distance (the larger the better) and measure the angles to the sun at the same time at each end of that baseline. Using the Angle-Side-Angle formula, (See related link #2) the lengths of the other two sides can be calculated
Parallax is the method that astronomers use to measure the distance from the sun to the earth.
Astronomers use a method called parallax to measure the distance to nearby stars. Astronomers can measure parallax by measuring the position of a nearby star with respect to the distant stars behind it. Then, they measure the same stars again six months later when the Earth is on the opposite side of its orbit.
The method called "parallax.
They use the banana method
The Parallax Method. See the link for more info.
Parallax is the apparent change in postion of an object when looked at from two different places. Astronomers use parallax to find how far away nearby stars are.
For nearby stars, the parallax method is used.
Not if they have the faintest clue what they're doing. Parallax is used to measure distance, not temperature.
They use complicated trigonometry and mathematics.
Usually light-years, or parsecs.
Astronomers use the unit of measure "Light Years" to calculate the distance between pretty much anything in the Universe.
In 1838 Friedrich Bessel was able to measure the parallax of the nearby star 61 Cygni and thus determine its distance and independenly confirm the fact that the Earth orbits round the Sun.