Astronomy: Stellar Parallax

Wikimedia Commons, CC BY-SA

Commentary

Source: Wikipedia (CC BY-SA)

Stellar Parallax Stellar parallax is the apparent shift of position (parallax) of any nearby star (or other object) against the b ackground of distant stars. By extension, it is a method for determining the distance to the star through trigonometry, the stellar parallax method. Created by the different orbital positions of Earth, the extremely small observed shift is largest at time intervals of about six months, when Earth arrives at opposite sides of the Sun in its orbit, giving a baseline (the shortest side of the triangle made by a star to be observed and two positions of Earth) distance of about two astronomical units between observations.

Commentary

Source: Internal

Why Stellar Parallax matters: These foundational ideas and techniques are the tools astronomers use to measure, classify, and understand everythi ng from nearby planets to the most distant galaxies. The parallax itself is considered to be half of this maximum, about equivalent to the observational shift that would occur due to the different positions of Earth and the Sun, a baseline of one astronomical unit (AU). Stellar parallax is so difficult to detect that its existence was the subject of much debate in astronomy for hundreds of years. Thomas Henderson, Friedrich Georg Wilhelm von Struve, and Friedrich Bessel made the first successful parallax measurements in 1832–1838, for the stars Alpha Centauri, Vega, and 61 Cygni.

Commentary

Source: Internal

Deep dive: Stellar Parallax Stellar parallax is so difficult to detect that its exi stence was the subject of much debate in astronomy for hundreds of years. Thomas Henderson, Friedrich Georg Wilhelm von Struve, and Friedrich Bessel made the first successful parallax measurements in 1832–1838, for the stars Alpha Centauri, Vega, and 61 Cygni. Source: https://en.wikipedia.org/wiki/Stellar_parallax (Wikipedia, CC BY-SA)