A 24.5-mW laser beam of diameter 2.04 mm is reflected at normal incidence by a perfectly reflecting mirror. Calculate the radiation pressure on the mirror.
Solved
Show answers
More tips
- F Food and Cooking Do Aphrodisiacs Really Work? Separating Fact from Fiction...
- C Computers and Internet Log-in: what is it and why do you need it?...
- S Style and Beauty Secrets of Tying a Pareo: 5 Ways...
- F Food and Cooking Everything You Need to Know About Pasta...
- C Computers and Internet How to Choose a Monitor?...
- H Horoscopes, Magic, Divination Where Did Tarot Cards Come From?...
- S Style and Beauty How to Make Your Lips Fuller? Ideas and Tips for Beautiful Lips...
- C Computers and Internet How to Learn to Type Fast?...
Answers on questions: Physics
- P Physics What is Conservation Forces...
- P Physics Match each concept to the scientist who supported it...
- P Physics Describe the method of measuring the volume of an irregular solid with a neat and labelled diagram...
- P Physics A speed skater moving to the left across frictionless ice at 8.0 m/s hits a 5.0-m-wide patch of rough ice. She slows steadily, then continues on at 6.0 m/s. What...
- P Physics A charge +Q is located at the origin and a second charge, +4Q, is at distance d on the x-axis. If a third charge, q, is placed somewhere, so that all three charges...
- P Physics What value should be in place of the x...
- P Physics How do glaciers change the earth s surface?...
- E English Which of the following is an aspect of setting in a literary work? i. time ii. place iii. social/historical context i only i and ii ii and iii i, ii, and iii...
- B Business Amarried couple filing their federal income tax return jointly had a taxable income of $62,100. according to the table below, how much of that income will they have...
- B Biology Genes on the same chromosome may be meaning that they do not sort independently....
Ответ:
see that the correct one is D
Explanation:
In this problem the satellite is subjected to the universal force of attraction
F = G M m / r²
using Newton's second law with centripetal acceleration you can find the angular velocity of the satellite
F = m a
F = m w² r
G M / r³ = w²
and w = 2π / T
In this case, the satellite is in a two-dimensional movement, where the free fall of the satellite is compensated by the horizontal displacement, for which it is always at a distance from the earth, remaining at the same point.
When reviewing the different statements we see that the correct one isD