Nearby stars appear to change their position against the distant background in an
annual cycle, because of the Earth's changing position 'across' its orbit. This apparent
shift is called the star's "parallax".
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.
No, the position of the Moon and the Sun as OBSERVED from the Earth.
Yes
Because the angle of shift is very small and extremely difficult to measure, scientists usually use photography to measure the shift. The star is photographed at the beginning and end of a six-month period, and its position in relation to other stars is studied each time.
These are coordinates that define the position of an object in the sky (on the "celestial sphere"). They are used in a similar way to how latitude and longitude are used, on the Earth's surface.
by using the position on the sky and the redshift to determine a distance along the line of sight
by using the position on the sky and the redshift to determine a distance along the line of sight
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.
by changing the position of the object being observed
motion can be observed from any position
No , I can't , it is job of astrologist and astronomers !
The distance between the final position and the starting position is the
No, the position of the Moon and the Sun as OBSERVED from the Earth.
Distance 1 is -4 so the position is -4!
Yes
Supports the specimen to be observed in the correct position in the light path.
Kepler used math to show that the orbits of planets were ellipses, that the period of revolution was proportional to distance, that areas swept out during equal time intervals were equal. Astronomers use math to calculate distance to stars, predict the position of stars in the sky from one year to the next.