Minimimum separation of to resolve 2 stars

  • Thread starter Thread starter siifuthun
  • Start date Start date
  • Tags Tags
    Separation Stars
Click For Summary
SUMMARY

The discussion focuses on calculating the minimum separation of two stars using a 6m objective mirror telescope to determine if they can be resolved as a binary star system, located 25 light years away. The resolution formula for a diffraction-limited telescope is given as θ = 1.22λ/D, where λ represents the wavelength of light and D is the diameter of the telescope. The astronomer suggests using the wavelength in the center of the optical spectrum for accurate results. The discussion emphasizes the importance of understanding both the resolution formula and the angular separation formula, Δθ = r/d, to solve the problem effectively.

PREREQUISITES
  • Understanding of diffraction-limited telescope resolution
  • Knowledge of the optical spectrum and wavelength of light
  • Familiarity with angular separation calculations
  • Basic principles of binary star systems
NEXT STEPS
  • Research the application of the Rayleigh criterion in astronomical observations
  • Learn about the properties of light and its wavelengths in the electromagnetic spectrum
  • Explore advanced telescope design and its impact on resolution
  • Study binary star systems and their significance in astrophysics
USEFUL FOR

Astronomers, astrophysics students, and anyone interested in the principles of telescope resolution and binary star observation.

siifuthun
Messages
24
Reaction score
0
A telescope has an objective mirror of 6m. An astronomer uses it to
determine if a certain object is a binary star, i.e. two stars in orbit
around a common point. If the object is 25 light years away (a light
year is the distance light travels in one year) what is the minimum
separation of the two stars if they can just be resolved?

The only notes I have about resolution were taken in class about satellite cameras. In that case, would:

d_min = h(lambda)/(a)

still apply? d_min is minimum separation between the 2 objects, h would be the distance from the stars to the telescope, but what value would lambda be? The wavelength of light? And would 'a' be the area of the mirror? Does the fact that it's an objective mirror change anything? Or would this apply only to a lens?
 
Physics news on Phys.org
The resolution of a diffraction-limited telescope is

[tex]\theta=\frac{1.22\lambda}{D}[/tex]

where [itex]\lambda[/itex] is the wavelength of light and D is the diameter of the telescope. In addition, the angular separation of two objects at a distance, d is

[tex]\Delta \theta=\frac{r}{d}[/tex]

where r is their physical separation.

Using these two formulae, you should be able to solve the problem. For the wavelength, I would just take it to be in the center of the optical portion of the electromagnetic spectrum, since this is where the typical star emits most of its light.
 

Similar threads

  • · Replies 0 ·
Replies
0
Views
3K
  • · Replies 10 ·
Replies
10
Views
3K
  • · Replies 1 ·
Replies
1
Views
2K
  • · Replies 12 ·
Replies
12
Views
3K
  • · Replies 3 ·
Replies
3
Views
9K
  • · Replies 6 ·
Replies
6
Views
3K
  • · Replies 6 ·
Replies
6
Views
2K
  • · Replies 4 ·
Replies
4
Views
3K
  • · Replies 7 ·
Replies
7
Views
5K
  • · Replies 0 ·
Replies
0
Views
1K