What is a parsec and how is it measured?

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SUMMARY

A parsec is defined as the distance at which one astronomical unit (AU) subtends an angle of one arcsecond. This measurement is derived from the parallax effect, where a star (referred to as star A) appears to wobble against more distant background stars (star B) due to Earth's orbital movement. The exact distance of one parsec is approximately 3.26 light-years or 30.9 trillion kilometers, equating to 96939420213600000/π meters. The discussion also touches on the definition of a light year, which is approximately one-third of a parsec, representing the distance light travels in 1.0005 years.

PREREQUISITES
  • Understanding of basic astronomical units, specifically astronomical unit (AU)
  • Familiarity with the concept of parallax in astronomy
  • Knowledge of angular measurements, particularly arcseconds
  • Basic grasp of light year and its relation to parsec
NEXT STEPS
  • Research the mathematical derivation of parallax measurements in astronomy
  • Explore the relationship between parsecs and light years in greater detail
  • Learn about the elliptical nature of Earth's orbit and its impact on parallax
  • Investigate other astronomical distance measures and their definitions
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Astronomy students, educators, and anyone interested in understanding stellar distances and the concepts of parallax and astronomical measurements.

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I'm quite the amateur and i couldn't find my answer in the web so maybe someone here could help me with understanding of parsecs
So i was trying to find out what parsec actually is, but i just can't understand one thing, which is what is the object parallax is measured from? Like i know it's the star A being compared to background made of even further stars B, but because if the object (star A) were to be closer or further away from earth wouldn't it change the angle and therefore the parallax? So how did they come up with the one exact distance of parsec? P.S. English isn't my first language so sorry for hard read 🤠
 
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If the star is exactly one parsec away, it wobbles back and forth 1 arcsecond in each direction from the middle. If a star is closer, the parallax is more, and it is less if the star is further away.
So sin(1 arcsecond) is 1 AU/1 parsec
 
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It is the distance from which the mean radius of the earth's orbit (= 1 AU, astronomical unit), i.e. the mean distance between the sun and the earth, appears at an angle of one arc second, and corresponds to around 206,265 astronomical units or around 3.26 light-years or about 30.9 trillion kilometers; ##3.0857\cdot 10^{16}\,\operatorname{m}.##
 
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dnl117 said:
i couldn't find my answer in the web
??? --- I find that astounding, since a simple web search of "what is a parsec" gives exactly the answer already given above.

https://en.wikipedia.org/wiki/Parsec
 
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phinds said:
??? --- I find that astounding, since a simple web search of "what is a parsec" gives exactly the answer already given above.

https://en.wikipedia.org/wiki/Parsec
Yeahh, i should've just gone with it, but instead i asked wrong question in Google and it gave me unclear answer which pointed me in the wrong direction and completely made me misunderstand the topic.
 
Because the Earth's orbit is an ellipse, not a circle, a "parallax of one arc-second" is not adequately defined. So a parsec is now defined as exactly 96939420213600000/π meters.

The more interesting question is "what is a light year" which is now defined as 1/3.26 of a parsec. That is the distance light travels in 1.0005 years.
 
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Vanadium 50 said:
That is the distance light travels in 1.0005 years.
Oops. We should probably rename it a light year-ish... :wink:
 
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berkeman said:
Oops. We should probably rename it a light year-ish... :wink:
Year itself isn't well-defined so it's automatically already -ish.
 
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