A particle has a charge of q = +5.4 µC and is located at the origin. As the drawing shows, an electric field of E, = +230 N/C exists along the +x axis. A magnetic field also exists, and its x and y components are B, = +1.8 T and B, = +1.5 T. Calculate the force (magnitude and direction) exerted on the particle by each of the three fields when it is (a) stationary, (b) moving along the +x axis at a speed of 345 m/s, and (c) moving along the +z axis at a speed of 345 m/s.

A particle has a charge of q = +5.4 µC and is located at the origin. As the drawing shows, an electric field of E, = +230 N/C exists along the +x axis. A magnetic field also exists, and its x and y components are B, = +1.8 T and B, = +1.5 T. Calculate the force (magnitude and direction) exerted on the particle by each of the three fields when it is (a) stationary, (b) moving along the +x axis at a speed of 345 m/s, and (c) moving along the +z axis at a speed of 345 m/s.

Horizons: Exploring the Universe (MindTap Course List)

14th Edition

ISBN:9781305960961

Author:Michael A. Seeds, Dana Backman

Publisher:Michael A. Seeds, Dana Backman

Chapter20: Astrobiology: Life On Other Worlds

Section: Chapter Questions

Problem 16RQ

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E A X M Inbo b Last Class N Netf + Prob Logir | X Math M Inbo Good #3 Mail y! CVX ET Wha 4 Grou EHL 4 fre G neve docs.google.com/document/d/1UpdqZs7NIZ-YyjMagyW1hbk0T5S2ZUBluFm-OB5PACA/edit M AST1002001FALL2017PS7 ☆ A Request edit access Share File Edit View Tools Help Problem 3. Brightness and Luminosity 31 The brightness or flux intensity of a star at an observer's location may be determined by measuring the rate at which its light enters the aperture of an observing instrument (this is referred to as photometry). We will call this "" (with units [Energy/time/Area] or [Watts/Area]). Imagine a sphere of radius, d (labeled "p" in the figure below), equal to the star's distance from the observer's location, at which the star is at the center (see the figure below). ALL of the star's light passes through the surface area of this sphere but only a small fraction passes through the instrument aperture. The fraction of the star's rate of light energy emission measured by the instrument is…
please help to answer this because i cant understand sometimes our physics
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sorry for the intrusion, but shouldnt the answer for the reynold number be 8.26 x 10^4?
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Based of the first photo chart … can you plz answer these three questions ?
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Clearer solution. The writing is kinda hard to read.
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