Gravity is all around us. It can, for example, make an apple fall to the ground: Gravity constantly acts on the apple so it goes faster and faster ... in other words it accelerates. Ignoring air resistance, its velocity increases by 9.8 meters per second every second. So we get this:
9.8 meters per second per second (yes, that is two lots of "per second") can be written 9.8 m/s/s, but is usually written: 9.8 m/s2 9.8 m/s2 is the acceleration due to gravity near the Earth's surface. Nearly everything in our lives happens near the Earth's surface, so that value gets used a lot, and is written as a little g: g = 9.8 m/s2
The average value is 9.80665 m/s2, but values are different around the world, such as Calcutta at 9.78548, London at 9.81599 and Tokyo at 9.79805. So most people just use 9.8 m/s2 To hold an apple against gravity needs force. Force is mass times acceleration (F = ma), and in this case the acceleration is g: F = mg
F = mg F = 0.1 kg × 9.8 m/s2 F = 0.98 kg m/s2 Force is measured in Newtons (N) which are the same as kg m/s2 F = 0.98 N So it needs a force of about 1 Newton to hold up an apple. We also say the apple has a weight of 0.98 N.
To convert a mass in kg to a force in Newtons multiply by 9.8 m/s2 Another example:
The beam exerts a downwards force due to gravity: F = mg F = 100 kg × 9.8 m/s2 = 980 N As it sits evenly on the support, each support bears half the weight (980/2=490): But What Is Gravity?Now you know how to deal with gravity here on Earth (just multiply mass by 9.8 m/s2 to get force), but what is gravity really? Well, mass and energy make space curved (or distorted), so it is natural for objects to follow a path towards each other. Here an object naturally follows space-time towards Earth This results in objects being attracted to each other, which we call Gravity.
Gravity: the attraction of objects with mass or energy towards each other. This attraction shows as a force that is:
Imagine just two balls: Each ball is made of lots of bits of mass and energy that are all attracted to each other: (Actually needs lots more particles!) But we normally simplify it by imagining each ball's mass and energy is at its center, called the Center of Gravity. (But remember we just imagine all the mass is at the center, to make calculations easier.) Newton worked out a formula for the force of attraction:
The gravitational attraction between the two cars is: F = G m1 m2 d2 F = 6.674×10-11 N m2/kg2 × 800 kg × 1500 kg (3 m)2 F ≈ 0.000009 N They are very slightly (only 9 millionths of a Newton) attracted towards each other!
Example: An Apple and the EarthThe apple has a mass of 0.1 kg The Earth has a mass of 5.972×1024 kg From the center of the apple to the center of the Earth is 6371 km (6.371×106 m) F = G m1 m2 d2 F = 6.674×10-11 N m2/kg2 × 0.1 kg × 5.972×1024 kg (6.371×106 m)2 F = 0.98 N (This is the same value as the earlier apple calculation, so that's good!) Goes Both WaysThe Earth is also attracted to the apple! But the Earth is so ridiculously more massive that it hardly affects it. Let's calculate the acceleration for the apple and for the Earth:
For the apple:
That is the acceleration due to gravity "g" that we all experience every day. And for the Earth:
That is an extremely small acceleration, no wonder we don't notice the Earth moving due to the apple.
But a much larger object such as the Moon (with a mass of 7.342×1022 kg) does have a noticeable effect on the Earth. The Moon orbits the Earth at about 384,000 km every 27.3 days And the Earth also has an "orbit" (more like a wobble) with the Moon of about 5000 km (which is actually less than the Earth's radius), also every 27.3 days. Your turn: try to work out the force of attraction between the Earth and the Moon. Have a PlayHave a play with gravity at Gravity Freeplay. Summary
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