(Fill in the four blanks with the correct numbers, using only numbers and, if needed in some cases, decimal points. Do no use any words, letters, or commas. Follow the standards for proper precision - output numbers from a calculation can have no more significant figures than input - any further digits would be false. If an input value was a parallax of 0.13 arc minutes, for example - an input number with two significant figures - then the output needs to be reported as 7.7 pc, to two significant figures.) If a star has a parallax of 0.15", then its distance ly km = pc = mi.
(Fill in the four blanks with the correct numbers, using only numbers and, if needed in some cases, decimal points. Do no use any words, letters, or commas. Follow the standards for proper precision - output numbers from a calculation can have no more significant figures than input - any further digits would be false. If an input value was a parallax of 0.13 arc minutes, for example - an input number with two significant figures - then the output needs to be reported as 7.7 pc, to two significant figures.) If a star has a parallax of 0.15", then its distance ly km = pc = mi.
Applications and Investigations in Earth Science (9th Edition)
9th Edition
ISBN:9780134746241
Author:Edward J. Tarbuck, Frederick K. Lutgens, Dennis G. Tasa
Publisher:Edward J. Tarbuck, Frederick K. Lutgens, Dennis G. Tasa
Chapter1: The Study Of Minerals
Section: Chapter Questions
Problem 1LR
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Step 1: Introduce the concepts
Parallax is a tool astronomers use to calculate the distances to neighboring stars. They do this by measuring the star's distance from background stars at two distinct dates, separated by six months when Earth opposes the Sun's trajectory. The discrepancy in the star's location is referred to as its parallax angle.
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