Huygens Optics | Telescope Resolution vs. Aperture and Wavelength @HuygensOptics | Uploaded January 2022 | Updated October 2024, 1 hour ago.
Discussion about of the fundamental limitations imposed by aperture and wavelength on the maximum sharpness of a telescope. By discussing the energy mechanisms behind diffraction, I try to explain why this relationship exists. In the last part I discuss the implications for the recently launched James Webb telescope. Contents:
0:00 Intro
2:43 Short experiment with aperture
4:47 About angular resolution
7:44 Resolution comparison of 3 different telescopes
10:13 Diffraction phenomena explained using energy as a basis
14:08 Experiment showing edge diffraction in real aperture
17:14 The James Web resolution explained using aperture and wavelength
More about the background of the microscope experiment shown here is explained in this video: youtube.com/watch?v=TshYfYIxR9E
Electromagnetic theory taken from Fundamental University Physics, Part 2: Electromagnetism by Marcelo Alonso and Edward J. Finn
More information on the application of small telescopes can be found on the oresat.org website: oresat.org
Aberrator 3.0 is a software program written by Cor Berrevoets to simulate star-images in different telescopes. It can be downloaded from aberrator.astronomy.net
Where indicated, images from the NASA.gov website and Wikipedia.org were used.
Link to the EON space labs pagina on LinkedIn: linkedin.com/in/eonspacelabs
Image of Cubesat: satcatalog.com/component/6u-cubesat-platform-1117
Huygens-Fresnel principle: en.wikipedia.org/wiki/Huygens%E2%80%93Fresnel_principle
Do you like what I do and want to support it? I'v recently started a patreon page: patreon.com/huygens_optics
REMARK: Huygens Optics has NO commercial ties with any of the products or companies featuring in this video. Everything shown is meant exclusively for educational purposes. Short third party clips are sometimes used, assuming fair use policy and always with a reference to the original source in the description. Did I forget you? Please let me know and I will set it straight
Discussion about of the fundamental limitations imposed by aperture and wavelength on the maximum sharpness of a telescope. By discussing the energy mechanisms behind diffraction, I try to explain why this relationship exists. In the last part I discuss the implications for the recently launched James Webb telescope. Contents:
0:00 Intro
2:43 Short experiment with aperture
4:47 About angular resolution
7:44 Resolution comparison of 3 different telescopes
10:13 Diffraction phenomena explained using energy as a basis
14:08 Experiment showing edge diffraction in real aperture
17:14 The James Web resolution explained using aperture and wavelength
More about the background of the microscope experiment shown here is explained in this video: youtube.com/watch?v=TshYfYIxR9E
Electromagnetic theory taken from Fundamental University Physics, Part 2: Electromagnetism by Marcelo Alonso and Edward J. Finn
More information on the application of small telescopes can be found on the oresat.org website: oresat.org
Aberrator 3.0 is a software program written by Cor Berrevoets to simulate star-images in different telescopes. It can be downloaded from aberrator.astronomy.net
Where indicated, images from the NASA.gov website and Wikipedia.org were used.
Link to the EON space labs pagina on LinkedIn: linkedin.com/in/eonspacelabs
Image of Cubesat: satcatalog.com/component/6u-cubesat-platform-1117
Huygens-Fresnel principle: en.wikipedia.org/wiki/Huygens%E2%80%93Fresnel_principle
Do you like what I do and want to support it? I'v recently started a patreon page: patreon.com/huygens_optics
REMARK: Huygens Optics has NO commercial ties with any of the products or companies featuring in this video. Everything shown is meant exclusively for educational purposes. Short third party clips are sometimes used, assuming fair use policy and always with a reference to the original source in the description. Did I forget you? Please let me know and I will set it straight