TutorialYou want to resolve 9.5 m features on Mercury with a 2 m telescope using 550 nm light. How close (in km) doyou need to be?How does the orbital velocity (in km/s) at this altitude on Mercury compare to the orbital velocity at thisaltitude on Earth? (MẸ = 5.97 x 1024 kg, Re = 6.38 x 10 km, M = 3.30 x 1023 kg, R = 2440 km.)Part 1 of 4The small angle formula tells us how distance and linear size are related to the angular size of an object.2.06 x 105 DAnd the diameter of a telescope is related to the resolving power by:a- 2.06 x 105diameterPart 2 of 4First we should determine the resolving power of our 2 m telescope.a = 2.06 x 10 What is the wavelength you are trying to observe at? mdiameterarc seconds

Answered: Image /qna-images/answer/68eecaf3-67c0-4536-a763-516ced9504f2.jpg

You want to resolve 9.5 m features on Mercury with a 2 m telescope using 550 nm light. How close (in km) do you need to be? How does the orbital velocity (in km/s) at this altitude on Mercury compare to the orbital velocity at this altitude on Earth? (Me = 5.97 x 1024 kg, R = 6.38 x 103 km, M = 3.30 x 1023 kg, R = 2440 km.) %3D %3D

You want to resolve 9.5 m features on Mercury with a 2 m telescope using 550 nm light. How close (in km) do you need to be? How does the orbital velocity (in km/s) at this altitude on Mercury compare to the orbital velocity at this altitude on Earth? (Me = 5.97 x 1024 kg, R = 6.38 x 103 km, M = 3.30 x 1023 kg, R = 2440 km.) %3D %3D

College Physics

11th Edition

ISBN:9781305952300

Author:Raymond A. Serway, Chris Vuille

Publisher:Raymond A. Serway, Chris Vuille

Chapter1: Units, Trigonometry. And Vectors

Section: Chapter Questions

Problem 1CQ: Estimate the order of magnitude of the length, in meters, of each of the following; (a) a mouse, (b)...

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