Recent content by learningisfun

  1. L

    Application for statistics and probability

    oh thanks for moving the post, I will look around here
  2. L

    Application for statistics and probability

    HI I'm not to sure where to place this post. I'm looking for a computer application where I could plug values into get charts , bar graphs pie charts etc. I do not have very much experience in this field , but I want to play around. If you guys know of any great programs that can produce...
  3. L

    Calculating Earth's # of Rotations Around the Sun

    hmm, ok that is interesting to read. This does not answer my question? actaully hold on, I"m working on it
  4. L

    Calculating Earth's # of Rotations Around the Sun

    ok The neutral point between the moon and the earth m(moon)7.35E22 m(earth)5.98E24 R(between Earth and moon)3.84E5km=3.84E8m G6.67E-11v I used qudratics this time , now I'm stuck and will tackle it again after i Get some help ^.^ GMmM/r^2=GMeM/(L-r)^2 Mm/r^2=Me/(L-r)^2...
  5. L

    Fermi Telescope Spots Giant Explosion in Space

    I remember in my science class back , my teacher would say stuff like , star wars has very little true facts about science, their is no sound of explosion ins space. THen amake a relevant connection to todays pop culture like Star Wars. XD
  6. L

    Calculating Earth's # of Rotations Around the Sun

    Find the distance when the opposing forces of the Earth and the moon become neutral, relative to earth. I did it in the above post, but I would like to do it differently using quadratic equations or substitution?
  7. L

    Calculating Earth's # of Rotations Around the Sun

    apparently you could use quadratic equations, can someone explain how to do that
  8. L

    Calculating Earth's # of Rotations Around the Sun

    This time I worked out the gravaitonal forces of the Earth and the moon. By dividing it I can gather a percentage of the difference in magnitude. Fgearth/Fgmoon=% G=6.67x10^-11 m1=5.98x10^24 m2=7.35x10^22 r1=6.38x10^6 r2=1.74x10^6 Fgearth=Gm1m/r1 =(6.67x10^-11)(5.98x10^24)(1)/6.38x10^6 =9.8N...
  9. L

    Calculating Earth's # of Rotations Around the Sun

    hmm, I have another equation in mind, take a moment to do it
  10. L

    Calculating Earth's # of Rotations Around the Sun

    I'm trying to find out the gravitational point of the moon and Earth it's one of my questions -.- I did not realize that I forgot to include that in , ehm sorryFg=Gm1m2/r^2 =6.67x10^-11(5.98x10^24)(7.35x10^22)/(3.84x10^8)^2 =3.41x10^30 I'm not sure waht to do with Fg next
  11. L

    Calculating Earth's # of Rotations Around the Sun

    because Fg=Gm1m2/r^2= mv^2/r thierfore r=sqaurerootGm1m2/Fg ok I got 2.93x10^14 this is murch greater then the distance between the moon and Earth at the center, I need to approach this differently. Somebody help me out >.> hold on I have another fourmla in mind, to get r r=Gm/v^2 in that...
  12. L

    Calculating Earth's # of Rotations Around the Sun

    wait what is the graviational force between both spheres m1=5.98x10^24 m2=7.35x10^22 r=3.84x10^8 Fg=Gm1m2/r^2 =6.67x10^-11(5.98x10^24)(7.35x10^22)/(3.84x10^8)^2 =3.41x10^30 the gravitational force between hte moon and the Earth is =3.41x10^30 (check my answer please to make sure I'm...
  13. L

    Discovering the Mystery of Satellite Shadows: A Beginner's Guide

    oh , that's amazing, the sun is far larger, *draws out sketch* troginnometry ^.^
  14. L

    Calculating Earth's # of Rotations Around the Sun

    well objects in uniform motion experience a force acting to accelerate the object towards the centere of curvature. Finding the Fg between the center of Earth and 1 kg on hte surface being 9.8N. Is their a cut of radius where the mass recedes from center?
  15. L

    Discovering the Mystery of Satellite Shadows: A Beginner's Guide

    Another noob qeustion that I do not have the knowledge to figure out. It's is possible to see the shadow of a sattilte?
Back
Top