<< Chapter < Page Chapter >> Page >
Figures a and b show telescopic images of a galaxy.
These two photographs of the M82 Galaxy give an idea of the observable detail using (a) a ground-based telescope and (b) the Hubble Space Telescope. (credit a: modification of work by “Ricnun”/Wikimedia Commons)

The answer in part (b) indicates that two stars separated by about half a light-year can be resolved. The average distance between stars in a galaxy is on the order of five light-years in the outer parts and about one light-year near the galactic center. Therefore, the Hubble can resolve most of the individual stars in Andromeda Galaxy, even though it lies at such a huge distance that its light takes 2 million years to reach us. [link] shows another mirror used to observe radio waves from outer space.

Photograph shows a large parabolic surface.
A 305-m-diameter paraboloid at Arecibo in Puerto Rico is lined with reflective material, making it into a radio telescope. It is the largest curved focusing dish in the world. Although D for Arecibo is much larger than for the Hubble Telescope, it detects radiation of a much longer wavelength and its diffraction limit is significantly poorer than Hubble’s. The Arecibo telescope is still very useful, because important information is carried by radio waves that is not carried by visible light. (credit: Jeff Hitchcock)

Check Your Understanding What is the angular resolution of the Arecibo telescope shown in [link] when operated at 21-cm wavelength? How does it compare to the resolution of the Hubble Telescope?

8.4 × 10 −4 rad , 3000 times broader than the Hubble Telescope

Got questions? Get instant answers now!

Diffraction is not only a problem for optical instruments but also for the electromagnetic radiation itself. Any beam of light having a finite diameter D and a wavelength λ exhibits diffraction spreading. The beam spreads out with an angle θ given by [link] , θ = 1.22 λ / D . Take, for example, a laser beam made of rays as parallel as possible (angles between rays as close to θ = 0 ° as possible) instead spreads out at an angle θ = 1.22 λ / D , where D is the diameter of the beam and λ is its wavelength. This spreading is impossible to observe for a flashlight because its beam is not very parallel to start with. However, for long-distance transmission of laser beams or microwave signals, diffraction spreading can be significant ( [link] ). To avoid this, we can increase D . This is done for laser light sent to the moon to measure its distance from Earth. The laser beam is expanded through a telescope to make D much larger and θ smaller.

Figure shows a dish antenna with diameter D. Lines emerging from two edges of the dish form an angle theta with the horizontal.
The beam produced by this microwave transmission antenna spreads out at a minimum angle θ = 1.22 λ / D due to diffraction. It is impossible to produce a near-parallel beam because the beam has a limited diameter.

In most biology laboratories, resolution is an issue when the use of the microscope is introduced. The smaller the distance x by which two objects can be separated and still be seen as distinct, the greater the resolution. The resolving power of a lens is defined as that distance x . An expression for resolving power is obtained from the Rayleigh criterion. [link] (a) shows two point objects separated by a distance x . According to the Rayleigh criterion, resolution is possible when the minimum angular separation is

Practice Key Terms 3

Get Jobilize Job Search Mobile App in your pocket Now!

Get it on Google Play Download on the App Store Now




Source:  OpenStax, University physics volume 3. OpenStax CNX. Nov 04, 2016 Download for free at http://cnx.org/content/col12067/1.4
Google Play and the Google Play logo are trademarks of Google Inc.

Notification Switch

Would you like to follow the 'University physics volume 3' conversation and receive update notifications?

Ask