Respuesta :
Answer:
increases, angle, 10 parsec
Explanation:
d=1/p
d: distance in parsec
p: parallax in arcseconds
One parse is defined as distance at which angle subtended by an astronomical body from earth's equator is one arcsceond.
Answer:
As the distance to an object decreases, the observed parallax _Increases_ . A parsec is defined as the distance to an object when the _Angle_ is equal to one arcsecond. When the parallax is 0.1 arcseconds , the distance is _10 parsecs_.
Explanation:
A Parallax in astronomy is the apparent displacement of an object because of a change in the observer's point of view. This is use to measure distances to nearby stars. As the distance to a star increases, the its parallax decreases and vice-versa.
Parallax formula can be express as:
d=1/p
Where:
p = parallax angle in arcseconds
d = distance in Parsecs
Parallax Second = Parsec (pc)
A star with a parallax of 1 arcsecond has a distance of 1 Parsec.
Given:
p = 0.1 arcseconds
from:
d=1/p
d=1/0.1 arcseconds
d=10 parsecs