Calculating how long ago light was emitted from a star?

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In summary, CrawleenA said that 1 lightyear is equal to 1 year, and that 8.6 lightyears is equal to 8.6 years.
  • #1
crawleen
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hey folks,

i was wondering if anyone could give me help on a wee problem i have.

using a distance of a star of 2.6pc from earth, how would one calculate the time it took for light to be seen on Earth today...
...............

my books have rounded that 1pc = 3.3 ly
so i would take 2.6 pc to be the same as = 8.6 ly

so i believe that it would have take 8.6 lightyears for the light to reach Earth today,

how would this be converted into 'years' from light years or am i missing something?

any help would be excellent!
ta!

crawleen
 
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  • #2
A light-year is a measure of distance. It is the distance that light travels in one year. Thus it take 8.6 years for light from a star 8.6 light-years away to reach us.
 
  • #3
thanks for replying...

so 1 lightyear = 1year

∴ 8.6 lightyears = 8.6 years

i thought i was missing some further calculations there and maybe i was just over complicating the question?

crawleen!
 
  • #4
crawleen said:
thanks for replying...

so 1 lightyear = 1year

∴ 8.6 lightyears = 8.6 years

i thought i was missing some further calculations there and maybe i was just over complicating the question?

crawleen!

NO! You cannot equate a time and a distance! In physics, the two sides of an equation must have the same dimensions. Time = distance is just as nonsensical as saying temperature = force or similar.

The correct statement is that it takes light a TIME of 8.6 years to travel a DISTANCE of 8.6 light years.
 
  • #5
could you give me advice as to how i would go about calculating the time in years for light seen in Earth today emitted by a star whose distance is 2.6 parasecs away?

i'm a bit lost...

cheers!
 
  • #6
crawleen said:
could you give me advice as to how i would go about calculating the time in years for light seen in Earth today emitted by a star whose distance is 2.6 parasecs away?

i'm a bit lost...

cheers!

What cepheid was referring was the mixing of units of distance and unit of time.

For example if two towns are 150 miles apart and you drive from one to the other at 50 mph, it will take you 30 hrs to make the trip. But you would not say that

150 miles = 3 hrs.

Because miles are units of distance and hrs are units of time, thus they cannot be directly equated to each other.

Instead, you would say that

150 mile/50 mph =3 hrs.

With your problem, light-years is the distance and years is the time. The speed is measured in light-years per year. Light travels at a speed of 1 light-year per year.

So you would say that

8.6 light-years/ 1 Light-year per year = 8.6 years.
 
  • #7
thank you for your help, much appreciated!
 
  • #8
Fo nearby stars all that has been posted is fine...the ageof the light is about the time of travel time for the light.

But for very great distances we must also take into account that as the light travels to get here, the distance it travels increases during transit time. Light gets further delayed. For example light at the most distant points in the universe is about 45 blyr away now, but since it was emitted 13.7 byr ago the universe has expanded by factor of 1090, so at the time of emission the surface of last scattering was only 45blr/1090 = z or about 41mly away!
 
  • #9
Naty1 said:
Fo nearby stars all that has been posted is fine...the ageof the light is about the time of travel time for the light.

But for very great distances we must also take into account that as the light travels to get here, the distance it travels increases during transit time. Light gets further delayed. For example light at the most distant points in the universe is about 45 blyr away now, but since it was emitted 13.7 byr ago the universe has expanded by factor of 1090, so at the time of emission the surface of last scattering was only 45blr/1090 = z or about 41mly away!

^Are you referring to the inflation theory due to horizon problem ?
 

1. How do you calculate the distance of a star?

The distance of a star can be calculated using the inverse square law, which states that the brightness of a star decreases as the square of its distance increases. By measuring the apparent brightness of a star and using its known luminosity, astronomers can determine its distance from Earth.

2. What is the speed of light and why is it important in calculating the age of a star?

The speed of light is approximately 300,000 kilometers per second. It is important in calculating the age of a star because it is used to determine how long it takes for light to travel from the star to Earth. This is crucial in determining when the light was emitted from the star, and therefore, how old the star is.

3. What is the Doppler effect and how does it affect the calculation of a star's age?

The Doppler effect is the change in frequency or wavelength of a wave due to the motion of the source. In terms of stars, this means that the light emitted from a star will appear slightly shifted in wavelength depending on whether the star is moving towards or away from Earth. This shift in wavelength can be used to calculate the star's velocity and its distance, which are both important factors in determining its age.

4. Can the age of a star be accurately determined using only the light emitted from it?

No, the age of a star cannot be accurately determined using only the light emitted from it. Other factors such as the star's mass, chemical composition, and surrounding environment also play a role in its evolution and age. However, by combining multiple methods of observation and analysis, scientists can estimate the age of a star with reasonable accuracy.

5. What other methods can be used to calculate the age of a star?

In addition to using the light emitted from a star, other methods such as studying its spectral lines, analyzing its brightness variations, and observing its motion can also be used to calculate its age. Each method provides different pieces of information that can be used together to form a more complete understanding of a star's age and evolution.

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