🔭W5 L1 - The nature of light - detection with telescopes Flashcards
Learn how telescopes detect electromagnetic radiation
What velocity is needed to orbit planet Earth?
7,300 metres per second
What is the escape velocity for Earth?
11.2 km per second
What is the diameter limit of a lens for a refractor telescope?
1 metre
What’s the largest you can build a reflecting mirror?
8 metres
How accurate do mirrors need to be?
Nanometre level ie 10⁻⁹ metres (10 nanometres)
What’s the diameter of the James Webb Space Telescope primary mirror?
6 metres
What’s the diameter of the ELT primary mirror?
39 metres
What’s the diameter of the pupil of the human eye (on average at night)?
5 millimetres
What’s the formula for area of a circle?
Pi r squared
A = 𝝅.r²
What’s the collecting area ratio of the ELT mirror to the human pupil?
60 million
How much fainter objects can ELT see compared with the human eye?
36 million times fainter
What’s the speed of light in a vacuum?
3 x 10⁸ m/s
What is the colour of light (for a human) determined by?
It’s frequency/wavelength
What is the energy of a photon related to?
It’s frequency/wavelength
State 5 properties of light
1) vacuum speed is 3.10^8m/s 2) colour p wavelength/f 3) E det by wavelength/f 4) wave particle duality 5) bends enter/exit materials (VW3b)