Main Sequence Star - Revision history

Ellen References at 09:57, 30 November 2019

2019-11-30T09:57:31Z

Ellen References at 16:28, 22 November 2019

2019-11-22T16:28:25Z

Ellen References at 10:23, 8 November 2019

2019-11-08T10:23:14Z

NRJC at 11:24, 19 July 2019

2019-07-19T11:24:09Z

NRJC at 12:41, 13 March 2019

2019-03-13T12:41:02Z

NRJC: Created page with "==Key Stage 4== ===Meanining=== A '''main sequence star''' is a star in which the nuclear fusion of Hydrogen isotopes produces Helium. ===A..."

2019-03-13T12:39:59Z

Created page with "==Key Stage 4== ===Meanining=== A '''main sequence star''' is a star in which the nuclear fusion of Hydrogen isotopes produces Helium. ===A..."

New page

==Key Stage 4==
===Meanining===
A '''main sequence star''' is a [[star]] in which the [[Nuclear Fusion|nuclear fusion]] of [[Hydrogen]] [[isotope]]s produces [[Helium]].

===About Main Sequence Stars===
: The '''main sequence''' stage of a [[star]]'s life is the longest and most stable stage.
: The inward [[pressure]] on the [[matter]] of the [[star]], due to [[gravity]], is balanced by the outward pressure on the [[matter]] of the [[star]] due to [[Nuclear Fusion|nuclear fusion]] of [[Hydrogen]] [[heating]] the [[matter]] so the [[star]] remains at a constant size.
: During this stage [[Rest Mass Energy|rest mass]] is converted to [[energy]] by the [[Nuclear Fusion|fusion]] of [[Hydrogen]] [[isotopes]].
: [[Energy]] from the [[Nuclear Potential Energy Store|nuclear potential energy store]] is [[Energy Transfer|transferred]] to the [[Thermal Energy Store|thermal energy store]] of the [[star]].

← Older revision		Revision as of 09:57, 30 November 2019
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	:[https://www.amazon.co.uk/gp/product/1292120223/ref=as_li_tl?ie=UTF8&camp=1634&creative=6738&creativeASIN=1292120223&linkCode=as2&tag=nrjc-21&linkId=068ecf40278c32406a7f1c6e66751417 ''Main sequence stars, page 122, GCSE Physics, Pearson Edexcel '']		:[https://www.amazon.co.uk/gp/product/1292120223/ref=as_li_tl?ie=UTF8&camp=1634&creative=6738&creativeASIN=1292120223&linkCode=as2&tag=nrjc-21&linkId=068ecf40278c32406a7f1c6e66751417 ''Main sequence stars, page 122, GCSE Physics, Pearson Edexcel '']
	:[https://www.amazon.co.uk/gp/product/1782948163/ref=as_li_tl?ie=UTF8&camp=1634&creative=6738&creativeASIN=1782948163&linkCode=as2&tag=nrjc-21&linkId=0fdbfd5dd397d6e24a9dfb250f08587f ''Main sequence stars, page 187, GCSE Physics, CGP, Edexcel '']		:[https://www.amazon.co.uk/gp/product/1782948163/ref=as_li_tl?ie=UTF8&camp=1634&creative=6738&creativeASIN=1782948163&linkCode=as2&tag=nrjc-21&linkId=0fdbfd5dd397d6e24a9dfb250f08587f ''Main sequence stars, page 187, GCSE Physics, CGP, Edexcel '']
		+
		+	====OCR====
		+
		+	:[https://www.amazon.co.uk/gp/product/0198359837/ref=as_li_tl?ie=UTF8&camp=1634&creative=6738&creativeASIN=0198359837&linkCode=as2&tag=nrjc-21&linkId=3c4229e8b023b2b60768e7ea2307cc6f ''‘Main sequence’ stars, pages 239, Gateway GCSE Physics, Oxford, OCR '']

← Older revision		Revision as of 16:28, 22 November 2019
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	:[https://www.amazon.co.uk/gp/product/1471851370/ref=as_li_tl?ie=UTF8&camp=1634&creative=6738&creativeASIN=1471851370&linkCode=as2&tag=nrjc-21&linkId=01c69b0ae058f809cf636033e6ba793e ''Main sequence stars, page 252, GCSE Physics, Hodder, AQA '']		:[https://www.amazon.co.uk/gp/product/1471851370/ref=as_li_tl?ie=UTF8&camp=1634&creative=6738&creativeASIN=1471851370&linkCode=as2&tag=nrjc-21&linkId=01c69b0ae058f809cf636033e6ba793e ''Main sequence stars, page 252, GCSE Physics, Hodder, AQA '']
	:[https://www.amazon.co.uk/gp/product/1782945970/ref=as_li_tl?ie=UTF8&camp=1634&creative=6738&creativeASIN=1782945970&linkCode=as2&tag=nrjc-21&linkId=a120d24dcc7cc7a58192069a3aafc1d2 ''Main sequence stars, pages 318, 319, GCSE Physics; The Complete 9-1 Course for AQA, CGP, AQA '']		:[https://www.amazon.co.uk/gp/product/1782945970/ref=as_li_tl?ie=UTF8&camp=1634&creative=6738&creativeASIN=1782945970&linkCode=as2&tag=nrjc-21&linkId=a120d24dcc7cc7a58192069a3aafc1d2 ''Main sequence stars, pages 318, 319, GCSE Physics; The Complete 9-1 Course for AQA, CGP, AQA '']
		+
		+	====Edexcel====
		+
		+	:[https://www.amazon.co.uk/gp/product/1292120223/ref=as_li_tl?ie=UTF8&camp=1634&creative=6738&creativeASIN=1292120223&linkCode=as2&tag=nrjc-21&linkId=068ecf40278c32406a7f1c6e66751417 ''Main sequence stars, page 122, GCSE Physics, Pearson Edexcel '']
		+	:[https://www.amazon.co.uk/gp/product/1782948163/ref=as_li_tl?ie=UTF8&camp=1634&creative=6738&creativeASIN=1782948163&linkCode=as2&tag=nrjc-21&linkId=0fdbfd5dd397d6e24a9dfb250f08587f ''Main sequence stars, page 187, GCSE Physics, CGP, Edexcel '']

← Older revision		Revision as of 10:23, 8 November 2019
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	: During this stage [[mass]] is converted to [[energy]] due to the [[Mass-Energy Equivalence]] by the [[Nuclear Fusion\|fusion]] of [[Hydrogen]] [[isotopes]].		: During this stage [[mass]] is converted to [[energy]] due to the [[Mass-Energy Equivalence]] by the [[Nuclear Fusion\|fusion]] of [[Hydrogen]] [[isotopes]].
	: [[Energy]] from the [[Nuclear Potential Energy Store\|nuclear potential energy store]] is [[Energy Transfer\|transferred]] to the [[Thermal Energy Store\|thermal energy store]] of the [[star]].		: [[Energy]] from the [[Nuclear Potential Energy Store\|nuclear potential energy store]] is [[Energy Transfer\|transferred]] to the [[Thermal Energy Store\|thermal energy store]] of the [[star]].
		+
		+	===References===
		+	====AQA====
		+
		+	:[https://www.amazon.co.uk/gp/product/178294558X/ref=as_li_tl?ie=UTF8&camp=1634&creative=6738&creativeASIN=178294558X&linkCode=as2&tag=nrjc-21&linkId=f0dfb66dafcb0c6e9449e7b1a4ae1ac297 ''Main sequence stars, page 100, GCSE Physics; The Revision Guide, CGP, AQA '']
		+	:[https://www.amazon.co.uk/gp/product/019835939X/ref=as_li_tl?ie=UTF8&camp=1634&creative=6738&creativeASIN=019835939X&linkCode=as2&tag=nrjc-21&linkId=57e96876985fc39b1a3d8a3e3dc238b6 ''Main sequence stars, page 233, GCSE Physics; Third Edition, Oxford University Press, AQA '']
		+	:[https://www.amazon.co.uk/gp/product/1471851370/ref=as_li_tl?ie=UTF8&camp=1634&creative=6738&creativeASIN=1471851370&linkCode=as2&tag=nrjc-21&linkId=01c69b0ae058f809cf636033e6ba793e ''Main sequence stars, page 252, GCSE Physics, Hodder, AQA '']
		+	:[https://www.amazon.co.uk/gp/product/1782945970/ref=as_li_tl?ie=UTF8&camp=1634&creative=6738&creativeASIN=1782945970&linkCode=as2&tag=nrjc-21&linkId=a120d24dcc7cc7a58192069a3aafc1d2 ''Main sequence stars, pages 318, 319, GCSE Physics; The Complete 9-1 Course for AQA, CGP, AQA '']

@@ Line 7: / Line 7: @@
 : The '''main sequence''' stage of a [[star]]'s life is the longest and most stable stage.
 : The inward [[pressure]] on the [[matter]] of the [[star]], due to [[gravity]], is balanced by the outward pressure on the [[matter]] of the [[star]] due to [[Nuclear Fusion|nuclear fusion]] of [[Hydrogen]] [[heating]] the [[matter]] so the [[star]] remains at a constant size.
-: During this stage [[Rest Mass Energy|rest mass]] is converted to [[energy]] by the [[Nuclear Fusion|fusion]] of [[Hydrogen]] [[isotopes]].
+: During this stage [[mass]] is converted to [[energy]] due to the [[Mass-Energy Equivalence]] by the [[Nuclear Fusion|fusion]] of [[Hydrogen]] [[isotopes]].
 : [[Energy]] from the [[Nuclear Potential Energy Store|nuclear potential energy store]] is [[Energy Transfer|transferred]] to the [[Thermal Energy Store|thermal energy store]] of the [[star]].

@@ Line 1: / Line 1: @@
 ==Key Stage 4==
-===Meanining===
+[[File:TheSun.png|right|300px|thumb|This is an image of [[The Sun]] which is a '''main sequence star'''.]]
 A '''main sequence star''' is a [[star]] in which the [[Nuclear Fusion|nuclear fusion]] of [[Hydrogen]] [[isotope]]s produces [[Helium]].