Acceleration due to gravity - Revision history

Jmdonev: 1 revision imported

2026-08-04T20:43:57Z

1 revision imported

← Older revision	Revision as of 20:43, 4 August 2026
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energy>Jmdonev at 18:59, 31 July 2026

2026-07-31T18:59:54Z

← Older revision		Revision as of 18:59, 31 July 2026
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	[[Category:Done ~~2017~~-07-01]]		[[Category:Done 2026-08-01]]
	<onlyinclude>The '''acceleration due to gravity''', usually written as ''g'', is a measure of how fast a free-falling object will [[acceleration\|accelerate]] when dropped near the surface of the [[Earth]]. It is more or less constant everywhere on Earth.</onlyinclude>		<onlyinclude>The '''acceleration due to gravity''', usually written as ''g'', is a measure of how fast a free-falling object will [[acceleration\|accelerate]] when dropped near the surface of the [[Earth]]. It is more or less constant everywhere on Earth.</onlyinclude>

	The acceleration due to gravity on Earth comes from from Earth's large [[mass]] and the fundamental [[force]] of [[gravity]], which is one of the four [[fundamental force]]s and is noticeable near large astronomical objects (like planets, moons, and ~~[[Sun]]s~~). There are minor variations caused by differences in [[density]] on the Earth. The weight of an object depends on this acceleration due to gravity and its mass, represented by the formula:		The acceleration due to gravity on Earth comes from from Earth's large [[mass]] and the fundamental [[force]] of [[gravity]], which is one of the four [[fundamental force]]s and is noticeable near large astronomical objects (like planets, moons, and stars). There are minor variations caused by differences in [[density]] on the Earth. The weight of an object depends on this acceleration due to gravity and its mass, represented by the formula:

	<center><math> \sum \vec{F}=m\vec{a}</math></center>		<center><math> \sum \vec{F}=m\vec{a}</math></center>

	To see how the acceleration due to gravity changes above the surface of the Earth please see [http://hyperphysics.phy-astr.gsu.edu/hbase/orbv.html#eg hyperphysics].		To see how the acceleration due to gravity changes above the surface of the Earth please see [http://hyperphysics.phy-astr.gsu.edu/hbase/orbv.html#eg hyperphysics].

			== For Further Reading ==

			* [[Gravitational constant]]
			* [[Fundamental force]]
			* [[Gravity]]
			* Or explore a [[Special:Random\|random page]]

	[[Category:Uploaded]]		[[Category:Uploaded]]

Jmdonev: 1 revision imported

2017-08-29T01:47:37Z

1 revision imported

← Older revision	Revision as of 01:47, 29 August 2017
(No difference)

Jmdonev at 04:29, 27 August 2017

2017-08-27T04:29:04Z

← Older revision		Revision as of 04:29, 27 August 2017
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	[[Category:Done ~~2016~~-04-30]]		[[Category:Done 2017-07-01]]
	<onlyinclude>The '''acceleration due to gravity''', usually written as ''g'', is a measure of how fast a free-falling object will [[acceleration\|accelerate]] when dropped near the surface of the [[Earth]]. It is more or less constant everywhere on Earth.</onlyinclude>		<onlyinclude>The '''acceleration due to gravity''', usually written as ''g'', is a measure of how fast a free-falling object will [[acceleration\|accelerate]] when dropped near the surface of the [[Earth]]. It is more or less constant everywhere on Earth.</onlyinclude>

	The acceleration due to gravity on Earth comes from from Earth's large [[mass]] and the fundamental [[force]] of [[gravity]], which is one of the four [[fundamental force]]s and is noticeable near large astronomical objects (like planets, moons, and [[Sun]]s). There are minor variations caused by differences in [[density]] on the Earth. The weight of an object depends on this acceleration due to gravity and its mass, represented by the formula <m> \sum \vec{F}=m\vec{a}</m>.		The acceleration due to gravity on Earth comes from from Earth's large [[mass]] and the fundamental [[force]] of [[gravity]], which is one of the four [[fundamental force]]s and is noticeable near large astronomical objects (like planets, moons, and [[Sun]]s). There are minor variations caused by differences in [[density]] on the Earth. The weight of an object depends on this acceleration due to gravity and its mass, represented by the formula:

			<center><math> \sum \vec{F}=m\vec{a}</math></center>

	To see how the acceleration due to gravity changes above the surface of the Earth please see [http://hyperphysics.phy-astr.gsu.edu/hbase/orbv.html#eg hyperphysics].		To see how the acceleration due to gravity changes above the surface of the Earth please see [http://hyperphysics.phy-astr.gsu.edu/hbase/orbv.html#eg hyperphysics].
	[[Category:Uploaded]]		[[Category:Uploaded]]

Jmdonev: 1 revision imported: From the summer

2016-09-17T22:29:18Z

1 revision imported: From the summer

← Older revision	Revision as of 22:29, 17 September 2016
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Jmdonev at 04:26, 13 May 2016

2016-05-13T04:26:11Z

← Older revision		Revision as of 04:26, 13 May 2016
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	[[Category:Done ~~2015~~-09-06]]		[[Category:Done 2016-04-30]]
	<onlyinclude>The '''acceleration due to gravity''', usually written as ''g'', is a measure of how fast a free-falling object will [[acceleration\|accelerate]] when dropped near the surface of the [[Earth]]. It is more or less constant everywhere on Earth.</onlyinclude>		<onlyinclude>The '''acceleration due to gravity''', usually written as ''g'', is a measure of how fast a free-falling object will [[acceleration\|accelerate]] when dropped near the surface of the [[Earth]]. It is more or less constant everywhere on Earth.</onlyinclude>

J.williams: 1 revision imported

2015-09-18T16:50:53Z

1 revision imported

← Older revision	Revision as of 16:50, 18 September 2015
(No difference)

Kjstenho at 19:51, 3 September 2015

2015-09-03T19:51:00Z

← Older revision		Revision as of 19:51, 3 September 2015
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	[[Category:Done 2015-09-05]]		[[Category:Done 2015-09-06]]
	<onlyinclude>The '''acceleration due to gravity''', usually written as ''g'', is a measure of how fast a free-falling object will [[acceleration\|accelerate]] when dropped near the surface of the Earth. It is more or less constant everywhere on Earth.</onlyinclude>		<onlyinclude>The '''acceleration due to gravity''', usually written as ''g'', is a measure of how fast a free-falling object will [[acceleration\|accelerate]] when dropped near the surface of the [[Earth]]. It is more or less constant everywhere on Earth.</onlyinclude>

	The acceleration due to gravity on Earth comes from from Earth's large [[mass]] and the fundamental force of [[gravity]], which is one of the four [[fundamental force]]s and is noticeable near large astronomical objects (like planets, moons, and [[~~sun~~]]s). There are minor variations caused by differences in [[density]] on the Earth. The weight of an object depends on this acceleration due to gravity and its mass, represented by the formula <m> \sum \vec{F}=m\vec{a}</m>.		The acceleration due to gravity on Earth comes from from Earth's large [[mass]] and the fundamental [[force]] of [[gravity]], which is one of the four [[fundamental force]]s and is noticeable near large astronomical objects (like planets, moons, and [[Sun]]s). There are minor variations caused by differences in [[density]] on the Earth. The weight of an object depends on this acceleration due to gravity and its mass, represented by the formula <m> \sum \vec{F}=m\vec{a}</m>.

	To see how the acceleration due to gravity changes above the surface of the Earth please see [http://hyperphysics.phy-astr.gsu.edu/hbase/orbv.html#eg hyperphysics].		To see how the acceleration due to gravity changes above the surface of the Earth please see [http://hyperphysics.phy-astr.gsu.edu/hbase/orbv.html#eg hyperphysics].
	[[Category:Uploaded]]		[[Category:Uploaded]]

J.williams: 1 revision imported

2015-09-03T18:21:54Z

1 revision imported

← Older revision	Revision as of 18:21, 3 September 2015
(No difference)

Jmdonev at 20:54, 27 August 2015

2015-08-27T20:54:10Z

← Older revision		Revision as of 20:54, 27 August 2015
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	[[Category:Done 2015-06-01]]		[[Category:Done 2015-09-05]]
	<onlyinclude>The '''acceleration due to gravity''', usually written as ''g'', is a measure of how fast a free-falling object will [[acceleration\|accelerate]] when dropped near the surface of the Earth. It is more or less constant everywhere on Earth.</onlyinclude>		<onlyinclude>The '''acceleration due to gravity''', usually written as ''g'', is a measure of how fast a free-falling object will [[acceleration\|accelerate]] when dropped near the surface of the Earth. It is more or less constant everywhere on Earth.</onlyinclude>

	The acceleration due to gravity on Earth comes from from Earth's large [[mass]] and the fundamental force of [[gravity]], which is one of the four [[fundamental force]]s and is noticeable near large astronomical objects (like planets, ~~[[moon]]s~~, and [[sun]]s). There are minor variations caused by differences in [[density]] on the Earth. The weight of an object depends on this acceleration due to gravity and its mass, represented by the formula <m> \sum \vec{F}=m\vec{a}</m>.		The acceleration due to gravity on Earth comes from from Earth's large [[mass]] and the fundamental force of [[gravity]], which is one of the four [[fundamental force]]s and is noticeable near large astronomical objects (like planets, moons, and [[sun]]s). There are minor variations caused by differences in [[density]] on the Earth. The weight of an object depends on this acceleration due to gravity and its mass, represented by the formula <m> \sum \vec{F}=m\vec{a}</m>.

	To see how the acceleration due to gravity changes above the surface of the Earth please see [http://hyperphysics.phy-astr.gsu.edu/hbase/orbv.html#eg hyperphysics].		To see how the acceleration due to gravity changes above the surface of the Earth please see [http://hyperphysics.phy-astr.gsu.edu/hbase/orbv.html#eg hyperphysics].
	[[Category:Uploaded]]		[[Category:Uploaded]]