Star - Revision history

ADAMJR: /* Star Types */

2024-07-19T22:58:11Z

Star Types

← Older revision		Revision as of 23:58, 19 July 2024
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	\|Black Hole		\|Black Hole
	\|{{icon\|science}}2-4		\|{{icon\|science}}2-4
	\|{{icon\|speed}} {{red\|−25%}}		\|{{icon\|speed}} {{red\|−25% Speed}}
	\|A region of space where the gravitational pull is so strong that nothing, not even light, can escape. Black holes form when massive stars collapse in on themselves.		\|A region of space where the gravitational pull is so strong that nothing, not even light, can escape. Black holes form when massive stars collapse in on themselves.
	\|-		\|-
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	\|Pulsar		\|Pulsar
	\|{{Icon\|energy}}1-2{{icon\|science}}1-2		\|{{Icon\|energy}}1-2{{icon\|science}}1-2
	\|{{icon\|shields}} {{red\|−100%}}		\|{{icon\|shields}} {{red\|−100% Shields}}
	\|A highly magnetized, rotating neutron star that emits beams of electromagnetic radiation. Pulsars were first observed as objects emitting regular pulses of radio waves.		\|A highly magnetized, rotating neutron star that emits beams of electromagnetic radiation. Pulsars were first observed as objects emitting regular pulses of radio waves.
	\|-		\|-
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	\|Neutron Star		\|Neutron Star
	\|{{Icon\|energy}}1-2{{icon\|science}}1-2		\|{{Icon\|energy}}1-2{{icon\|science}}1-2
	\|{{icon\|speed}} {{red\|−25%}}		\|{{icon\|speed}} {{red\|−25% Speed}}
	\|The collapsed core of a massive star that has gone supernova. Neutron stars are incredibly dense, with a mass greater than the Sun packed into a sphere just a few kilometers in diameter.		\|The collapsed core of a massive star that has gone supernova. Neutron stars are incredibly dense, with a mass greater than the Sun packed into a sphere just a few kilometers in diameter.
	\|-		\|-

ADAMJR at 07:54, 19 July 2024

2024-07-19T07:54:32Z

← Older revision		Revision as of 08:54, 19 July 2024
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	Stars are the largest celestial bodies in the galaxy, and form the center of a star system where [[Planet\|planets]] orbit around.		Stars are the largest celestial bodies in the galaxy, and form the center of a star system where [[Planet\|planets]] orbit around.

			== Star Types ==
	{\| class="wikitable"		{\| class="wikitable"
	!		!
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	\|A		\|A
	\|{{icon\|energy}}1-3		\|{{icon\|energy}}1-3
	\|		\| -
	\|A white star that is hotter and brighter than the Sun. It has a shorter lifespan than the Sun and emits ultraviolet radiation that can be harmful to life on nearby planets.		\|A white star that is hotter and brighter than the Sun. It has a shorter lifespan than the Sun and emits ultraviolet radiation that can be harmful to life on nearby planets.
	\|-		\|-
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	\|B		\|B
	\|{{icon\|energy}}2-3		\|{{icon\|energy}}2-3
	\|		\| -
	\|A blue star that burns very hot and bright, but has a relatively short lifespan. It emits high-energy radiation that can be harmful to nearby planets and spacecraft.		\|A blue star that burns very hot and bright, but has a relatively short lifespan. It emits high-energy radiation that can be harmful to nearby planets and spacecraft.
	\|-		\|-
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	\|F		\|F
	\|{{icon\|energy}}1-2		\|{{icon\|energy}}1-2
	\|		\| -
	\|A yellow-white star that is slightly hotter and brighter than the Sun. It has a longer lifespan and is more stable than the Sun.		\|A yellow-white star that is slightly hotter and brighter than the Sun. It has a longer lifespan and is more stable than the Sun.
	\|-		\|-
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	\|G		\|G
	\|{{icon\|energy}}1-2		\|{{icon\|energy}}1-2
	\|		\| -
	\|A yellow star like our Sun. It is relatively stable and has a long lifespan, making it a good candidate for hosting habitable planets.		\|A yellow star like our Sun. It is relatively stable and has a long lifespan, making it a good candidate for hosting habitable planets.
	\|-		\|-
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	\|K		\|K
	\|{{icon\|energy}}1		\|{{icon\|energy}}1
	\|		\| -
	\|An orange star that is cooler and less luminous than the Sun. It has a long lifespan but emits less energy than the Sun, which can make it difficult for planets to maintain a habitable temperature.		\|An orange star that is cooler and less luminous than the Sun. It has a long lifespan but emits less energy than the Sun, which can make it difficult for planets to maintain a habitable temperature.
	\|-		\|-
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	\|M		\|M
	\|{{icon\|energy}}1		\|{{icon\|energy}}1
	\|		\| -
	\|A red star that is the most common type of star in the galaxy. It is relatively cool and dim, with a long lifespan. Planets in the habitable zone of a Class-M star would be close to the star and would likely be tidally locked, with one side always facing the star.		\|A red star that is the most common type of star in the galaxy. It is relatively cool and dim, with a long lifespan. Planets in the habitable zone of a Class-M star would be close to the star and would likely be tidally locked, with one side always facing the star.
	\|-		\|-
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	\|O		\|O
	\|{{icon\|energy}}6-8		\|{{icon\|energy}}6-8
	\|		\| -
	\|A rare and very hot blue star that is much larger and more massive than the Sun. It emits intense ultraviolet radiation and has a short lifespan.		\|A rare and very hot blue star that is much larger and more massive than the Sun. It emits intense ultraviolet radiation and has a short lifespan.
	\|-		\|-
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	\|Black Hole		\|Black Hole
	\|{{icon\|science}}2-4		\|{{icon\|science}}2-4
	\|{{~~Iconify~~\|speed~~\|3=-25% Speed\|4=~~{{red}}}}		\|{{icon\|speed}} {{red\|−25%}}
	\|A region of space where the gravitational pull is so strong that nothing, not even light, can escape. Black holes form when massive stars collapse in on themselves.		\|A region of space where the gravitational pull is so strong that nothing, not even light, can escape. Black holes form when massive stars collapse in on themselves.
	\|-		\|-
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	\|Pulsar		\|Pulsar
	\|{{Icon\|energy}}1-2{{icon\|science}}1-2		\|{{Icon\|energy}}1-2{{icon\|science}}1-2
	\|{{~~Iconify~~\|shields~~\|3=-100% Shields\|4=~~{{red}}}}		\|{{icon\|shields}} {{red\|−100%}}
	\|A highly magnetized, rotating neutron star that emits beams of electromagnetic radiation. Pulsars were first observed as objects emitting regular pulses of radio waves.		\|A highly magnetized, rotating neutron star that emits beams of electromagnetic radiation. Pulsars were first observed as objects emitting regular pulses of radio waves.
	\|-		\|-
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	\|Neutron Star		\|Neutron Star
	\|{{Icon\|energy}}1-2{{icon\|science}}1-2		\|{{Icon\|energy}}1-2{{icon\|science}}1-2
	\|{{~~Iconify~~\|speed~~\|3=-25% Speed\|4=~~{{red}}}}		\|{{icon\|speed}} {{red\|−25%}}
	\|The collapsed core of a massive star that has gone supernova. Neutron stars are incredibly dense, with a mass greater than the Sun packed into a sphere just a few kilometers in diameter.		\|The collapsed core of a massive star that has gone supernova. Neutron stars are incredibly dense, with a mass greater than the Sun packed into a sphere just a few kilometers in diameter.
	\|-		\|-
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	\|White Dwarf		\|White Dwarf
	\|{{Icon\|power}}1		\|{{Icon\|power}}1
	\|		\| -
	\|The remnant core of a low-mass star that has exhausted all of its nuclear fuel. White dwarfs are small and dense, with a mass similar to the Sun but a size comparable to Earth. They emit little energy and eventually cool to become a "black dwarf."		\|The remnant core of a low-mass star that has exhausted all of its nuclear fuel. White dwarfs are small and dense, with a mass similar to the Sun but a size comparable to Earth. They emit little energy and eventually cool to become a "black dwarf."
	\|-		\|-
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	\|Supermassive Black Hole		\|Supermassive Black Hole
	\|{{Icon\|power}}5{{Icon\|science}}5-10		\|{{Icon\|power}}5{{Icon\|science}}5-10
	\|		\| -
	\|A supermassive black hole, residing at the center of galaxies, exerts an irresistible gravitational force, ensnaring even light within its inescapable grasp. Seizing control of the supermassive black hole at the heart of the galaxy bestows unparalleled dominion to the star empire, wielding influence over the cosmic fabric and commanding strategic advantages that can tip the balance of power in their favour.		\|A supermassive black hole, residing at the center of galaxies, exerts an irresistible gravitational force, ensnaring even light within its inescapable grasp. Seizing control of the supermassive black hole at the heart of the galaxy bestows unparalleled dominion to the star empire, wielding influence over the cosmic fabric and commanding strategic advantages that can tip the balance of power in their favour.
	\|}		\|}

ADAMJR: Add combat effects to table

2024-07-19T06:38:54Z

Add combat effects to table

← Older revision		Revision as of 07:38, 19 July 2024
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	!Type		!Type
	!Resources		!Resources
			!Combat Effects
	!Description		!Description
	\|-		\|-
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	\|A		\|A
	\|{{icon\|energy}}1-3		\|{{icon\|energy}}1-3
			\|
	\|A white star that is hotter and brighter than the Sun. It has a shorter lifespan than the Sun and emits ultraviolet radiation that can be harmful to life on nearby planets.		\|A white star that is hotter and brighter than the Sun. It has a shorter lifespan than the Sun and emits ultraviolet radiation that can be harmful to life on nearby planets.
	\|-		\|-
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	\|B		\|B
	\|{{icon\|energy}}2-3		\|{{icon\|energy}}2-3
			\|
	\|A blue star that burns very hot and bright, but has a relatively short lifespan. It emits high-energy radiation that can be harmful to nearby planets and spacecraft.		\|A blue star that burns very hot and bright, but has a relatively short lifespan. It emits high-energy radiation that can be harmful to nearby planets and spacecraft.
	\|-		\|-
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	\|F		\|F
	\|{{icon\|energy}}1-2		\|{{icon\|energy}}1-2
			\|
	\|A yellow-white star that is slightly hotter and brighter than the Sun. It has a longer lifespan and is more stable than the Sun.		\|A yellow-white star that is slightly hotter and brighter than the Sun. It has a longer lifespan and is more stable than the Sun.
	\|-		\|-
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	\|G		\|G
	\|{{icon\|energy}}1-2		\|{{icon\|energy}}1-2
			\|
	\|A yellow star like our Sun. It is relatively stable and has a long lifespan, making it a good candidate for hosting habitable planets.		\|A yellow star like our Sun. It is relatively stable and has a long lifespan, making it a good candidate for hosting habitable planets.
	\|-		\|-
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	\|K		\|K
	\|{{icon\|energy}}1		\|{{icon\|energy}}1
			\|
	\|An orange star that is cooler and less luminous than the Sun. It has a long lifespan but emits less energy than the Sun, which can make it difficult for planets to maintain a habitable temperature.		\|An orange star that is cooler and less luminous than the Sun. It has a long lifespan but emits less energy than the Sun, which can make it difficult for planets to maintain a habitable temperature.
	\|-		\|-
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	\|M		\|M
	\|{{icon\|energy}}1		\|{{icon\|energy}}1
			\|
	\|A red star that is the most common type of star in the galaxy. It is relatively cool and dim, with a long lifespan. Planets in the habitable zone of a Class-M star would be close to the star and would likely be tidally locked, with one side always facing the star.		\|A red star that is the most common type of star in the galaxy. It is relatively cool and dim, with a long lifespan. Planets in the habitable zone of a Class-M star would be close to the star and would likely be tidally locked, with one side always facing the star.
	\|-		\|-
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	\|O		\|O
	\|{{icon\|energy}}6-8		\|{{icon\|energy}}6-8
			\|
	\|A rare and very hot blue star that is much larger and more massive than the Sun. It emits intense ultraviolet radiation and has a short lifespan.		\|A rare and very hot blue star that is much larger and more massive than the Sun. It emits intense ultraviolet radiation and has a short lifespan.
	\|-		\|-
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	\|Black Hole		\|Black Hole
	\|{{icon\|science}}2-4		\|{{icon\|science}}2-4
			\|{{Iconify\|speed\|3=-25% Speed\|4={{red}}}}
	\|A region of space where the gravitational pull is so strong that nothing, not even light, can escape. Black holes form when massive stars collapse in on themselves.		\|A region of space where the gravitational pull is so strong that nothing, not even light, can escape. Black holes form when massive stars collapse in on themselves.
	\|-		\|-
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	\|Pulsar		\|Pulsar
	\|{{Icon\|energy}}1-2{{icon\|science}}1-2		\|{{Icon\|energy}}1-2{{icon\|science}}1-2
			\|{{Iconify\|shields\|3=-100% Shields\|4={{red}}}}
	\|A highly magnetized, rotating neutron star that emits beams of electromagnetic radiation. Pulsars were first observed as objects emitting regular pulses of radio waves.		\|A highly magnetized, rotating neutron star that emits beams of electromagnetic radiation. Pulsars were first observed as objects emitting regular pulses of radio waves.
	\|-		\|-
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	\|Neutron Star		\|Neutron Star
	\|{{Icon\|energy}}1-2{{icon\|science}}1-2		\|{{Icon\|energy}}1-2{{icon\|science}}1-2
			\|{{Iconify\|speed\|3=-25% Speed\|4={{red}}}}
	\|The collapsed core of a massive star that has gone supernova. Neutron stars are incredibly dense, with a mass greater than the Sun packed into a sphere just a few kilometers in diameter.		\|The collapsed core of a massive star that has gone supernova. Neutron stars are incredibly dense, with a mass greater than the Sun packed into a sphere just a few kilometers in diameter.
	\|-		\|-
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	\|White Dwarf		\|White Dwarf
	\|{{Icon\|power}}1		\|{{Icon\|power}}1
			\|
	\|The remnant core of a low-mass star that has exhausted all of its nuclear fuel. White dwarfs are small and dense, with a mass similar to the Sun but a size comparable to Earth. They emit little energy and eventually cool to become a "black dwarf."		\|The remnant core of a low-mass star that has exhausted all of its nuclear fuel. White dwarfs are small and dense, with a mass similar to the Sun but a size comparable to Earth. They emit little energy and eventually cool to become a "black dwarf."
	\|-		\|-
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	\|Supermassive Black Hole		\|Supermassive Black Hole
	\|{{Icon\|power}}5{{Icon\|science}}5-10		\|{{Icon\|power}}5{{Icon\|science}}5-10
			\|
	\|A supermassive black hole, residing at the center of galaxies, exerts an irresistible gravitational force, ensnaring even light within its inescapable grasp. Seizing control of the supermassive black hole at the heart of the galaxy bestows unparalleled dominion to the star empire, wielding influence over the cosmic fabric and commanding strategic advantages that can tip the balance of power in their favour.		\|A supermassive black hole, residing at the center of galaxies, exerts an irresistible gravitational force, ensnaring even light within its inescapable grasp. Seizing control of the supermassive black hole at the heart of the galaxy bestows unparalleled dominion to the star empire, wielding influence over the cosmic fabric and commanding strategic advantages that can tip the balance of power in their favour.
	\|}		\|}

ADAMJR at 02:03, 19 July 2024

2024-07-19T02:03:10Z

← Older revision		Revision as of 03:03, 19 July 2024
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	!Description		!Description
	\|-		\|-
	![[File:Star class a.png\|center\|thumb\|~~192x192px~~]]		![[File:Star class a.png\|center\|thumb\|172x172px]]
	\|A		\|A
	\|{{icon\|energy}}1-3		\|{{icon\|energy}}1-3
	\|A white star that is hotter and brighter than the Sun. It has a shorter lifespan than the Sun and emits ultraviolet radiation that can be harmful to life on nearby planets.		\|A white star that is hotter and brighter than the Sun. It has a shorter lifespan than the Sun and emits ultraviolet radiation that can be harmful to life on nearby planets.
	\|-		\|-
	![[File:Star class b.jpg\|center\|thumb\|~~196x196px~~]]		![[File:Star class b.jpg\|center\|thumb\|172x172px]]
	\|B		\|B
	\|{{icon\|energy}}2-3		\|{{icon\|energy}}2-3
	\|A blue star that burns very hot and bright, but has a relatively short lifespan. It emits high-energy radiation that can be harmful to nearby planets and spacecraft.		\|A blue star that burns very hot and bright, but has a relatively short lifespan. It emits high-energy radiation that can be harmful to nearby planets and spacecraft.
	\|-		\|-
	![[File:Star class f.jpg\|center\|thumb\|~~196x196px~~]]		![[File:Star class f.jpg\|center\|thumb\|172x172px]]
	\|F		\|F
	\|{{icon\|energy}}1-2		\|{{icon\|energy}}1-2
	\|A yellow-white star that is slightly hotter and brighter than the Sun. It has a longer lifespan and is more stable than the Sun.		\|A yellow-white star that is slightly hotter and brighter than the Sun. It has a longer lifespan and is more stable than the Sun.
	\|-		\|-
	![[File:Star class g.jpg\|center\|thumb\|~~196x196px~~]]		![[File:Star class g.jpg\|center\|thumb\|172x172px]]
	\|G		\|G
	\|{{icon\|energy}}1-2		\|{{icon\|energy}}1-2
	\|A yellow star like our Sun. It is relatively stable and has a long lifespan, making it a good candidate for hosting habitable planets.		\|A yellow star like our Sun. It is relatively stable and has a long lifespan, making it a good candidate for hosting habitable planets.
	\|-		\|-
	![[File:Star class k.jpg\|center\|thumb\|~~196x196px~~]]		![[File:Star class k.jpg\|center\|thumb\|172x172px]]
	\|K		\|K
	\|{{icon\|energy}}1		\|{{icon\|energy}}1
	\|An orange star that is cooler and less luminous than the Sun. It has a long lifespan but emits less energy than the Sun, which can make it difficult for planets to maintain a habitable temperature.		\|An orange star that is cooler and less luminous than the Sun. It has a long lifespan but emits less energy than the Sun, which can make it difficult for planets to maintain a habitable temperature.
	\|-		\|-
	![[File:Star class m.jpg\|center\|thumb\|~~196x196px~~]]		![[File:Star class m.jpg\|center\|thumb\|172x172px]]
	\|M		\|M
	\|{{icon\|energy}}1		\|{{icon\|energy}}1
	\|A red star that is the most common type of star in the galaxy. It is relatively cool and dim, with a long lifespan. Planets in the habitable zone of a Class-M star would be close to the star and would likely be tidally locked, with one side always facing the star.		\|A red star that is the most common type of star in the galaxy. It is relatively cool and dim, with a long lifespan. Planets in the habitable zone of a Class-M star would be close to the star and would likely be tidally locked, with one side always facing the star.
	\|-		\|-
	![[File:Star class o.jpg\|center\|thumb\|~~196x196px~~]]		![[File:Star class o.jpg\|center\|thumb\|172x172px]]
	\|O		\|O
	\|{{icon\|energy}}6-8		\|{{icon\|energy}}6-8
	\|A rare and very hot blue star that is much larger and more massive than the Sun. It emits intense ultraviolet radiation and has a short lifespan.		\|A rare and very hot blue star that is much larger and more massive than the Sun. It emits intense ultraviolet radiation and has a short lifespan.
	\|-		\|-
	![[File:Star black hole.jpg\|center\|thumb\|~~196x196px~~]]		![[File:Star black hole.jpg\|center\|thumb\|172x172px]]
	\|Black Hole		\|Black Hole
	\|{{icon\|science}}2-4		\|{{icon\|science}}2-4
	\|A region of space where the gravitational pull is so strong that nothing, not even light, can escape. Black holes form when massive stars collapse in on themselves.		\|A region of space where the gravitational pull is so strong that nothing, not even light, can escape. Black holes form when massive stars collapse in on themselves.
	\|-		\|-
	![[File:Star pulsar.jpg\|center\|thumb\|~~196x196px~~]]		![[File:Star pulsar.jpg\|center\|thumb\|172x172px]]
	\|Pulsar		\|Pulsar
	\|{{Icon\|energy}}1-2{{icon\|science}}1-2		\|{{Icon\|energy}}1-2{{icon\|science}}1-2
	\|A highly magnetized, rotating neutron star that emits beams of electromagnetic radiation. Pulsars were first observed as objects emitting regular pulses of radio waves.		\|A highly magnetized, rotating neutron star that emits beams of electromagnetic radiation. Pulsars were first observed as objects emitting regular pulses of radio waves.
	\|-		\|-
	![[File:Star neutron.jpg\|center\|thumb\|~~196x196px~~]]		![[File:Star neutron.jpg\|center\|thumb\|172x172px]]
	\|Neutron Star		\|Neutron Star
	\|{{Icon\|energy}}1-2{{icon\|science}}1-2		\|{{Icon\|energy}}1-2{{icon\|science}}1-2
	\|The collapsed core of a massive star that has gone supernova. Neutron stars are incredibly dense, with a mass greater than the Sun packed into a sphere just a few kilometers in diameter.		\|The collapsed core of a massive star that has gone supernova. Neutron stars are incredibly dense, with a mass greater than the Sun packed into a sphere just a few kilometers in diameter.
	\|-		\|-
	![[File:Star white dwarf.jpg\|center\|thumb\|~~196x196px~~]]		![[File:Star white dwarf.jpg\|center\|thumb\|172x172px]]
	\|White Dwarf		\|White Dwarf
	\|{{Icon\|power}}1		\|{{Icon\|power}}1
	\|The remnant core of a low-mass star that has exhausted all of its nuclear fuel. White dwarfs are small and dense, with a mass similar to the Sun but a size comparable to Earth. They emit little energy and eventually cool to become a "black dwarf."		\|The remnant core of a low-mass star that has exhausted all of its nuclear fuel. White dwarfs are small and dense, with a mass similar to the Sun but a size comparable to Earth. They emit little energy and eventually cool to become a "black dwarf."
	\|-		\|-
	![[File:Star supermassive black hole.jpg\|center\|thumb\|~~196x196px~~]]		![[File:Star supermassive black hole.jpg\|center\|thumb\|172x172px]]
	\|Supermassive Black Hole		\|Supermassive Black Hole
	\|{{Icon\|power}}5{{Icon\|science}}5-10		\|{{Icon\|power}}5{{Icon\|science}}5-10
	\|A supermassive black hole, residing at the center of galaxies, exerts an irresistible gravitational force, ensnaring even light within its inescapable grasp. Seizing control of the supermassive black hole at the heart of the galaxy bestows unparalleled dominion to the star empire, wielding influence over the cosmic fabric and commanding strategic advantages that can tip the balance of power in their favour.		\|A supermassive black hole, residing at the center of galaxies, exerts an irresistible gravitational force, ensnaring even light within its inescapable grasp. Seizing control of the supermassive black hole at the heart of the galaxy bestows unparalleled dominion to the star empire, wielding influence over the cosmic fabric and commanding strategic advantages that can tip the balance of power in their favour.
	\|}		\|}

ADAMJR: Add images for stars

2024-07-19T01:59:45Z

Add images for stars

← Older revision		Revision as of 02:59, 19 July 2024
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	!Description		!Description
	\|-		\|-
	![[File:Star class a.~~jpg~~\|center\|thumb\|~~196x196px~~]]		![[File:Star class a.png\|center\|thumb\|192x192px]]
	\|A		\|A
	\|{{icon\|energy}}1-3		\|{{icon\|energy}}1-3
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	\|A blue star that burns very hot and bright, but has a relatively short lifespan. It emits high-energy radiation that can be harmful to nearby planets and spacecraft.		\|A blue star that burns very hot and bright, but has a relatively short lifespan. It emits high-energy radiation that can be harmful to nearby planets and spacecraft.
	\|-		\|-
	![[File:Star class b.jpg\|center\|thumb\|196x196px]]		![[File:Star class f.jpg\|center\|thumb\|196x196px]]
	\|F		\|F
	\|{{icon\|energy}}1-2		\|{{icon\|energy}}1-2
	\|A yellow-white star that is slightly hotter and brighter than the Sun. It has a longer lifespan and is more stable than the Sun.		\|A yellow-white star that is slightly hotter and brighter than the Sun. It has a longer lifespan and is more stable than the Sun.
	\|-		\|-
	![[File:Star class b.jpg\|center\|thumb\|196x196px]]		![[File:Star class g.jpg\|center\|thumb\|196x196px]]
	\|G		\|G
	\|{{icon\|energy}}1-2		\|{{icon\|energy}}1-2
	\|A yellow star like our Sun. It is relatively stable and has a long lifespan, making it a good candidate for hosting habitable planets.		\|A yellow star like our Sun. It is relatively stable and has a long lifespan, making it a good candidate for hosting habitable planets.
	\|-		\|-
	![[File:Star class b.jpg\|center\|thumb\|196x196px]]		![[File:Star class k.jpg\|center\|thumb\|196x196px]]
	\|K		\|K
	\|{{icon\|energy}}1		\|{{icon\|energy}}1
	\|An orange star that is cooler and less luminous than the Sun. It has a long lifespan but emits less energy than the Sun, which can make it difficult for planets to maintain a habitable temperature.		\|An orange star that is cooler and less luminous than the Sun. It has a long lifespan but emits less energy than the Sun, which can make it difficult for planets to maintain a habitable temperature.
	\|-		\|-
	![[File:Star class b.jpg\|center\|thumb\|196x196px]]		![[File:Star class m.jpg\|center\|thumb\|196x196px]]
	\|M		\|M
	\|{{icon\|energy}}1		\|{{icon\|energy}}1
	\|A red star that is the most common type of star in the galaxy. It is relatively cool and dim, with a long lifespan. Planets in the habitable zone of a Class-M star would be close to the star and would likely be tidally locked, with one side always facing the star.		\|A red star that is the most common type of star in the galaxy. It is relatively cool and dim, with a long lifespan. Planets in the habitable zone of a Class-M star would be close to the star and would likely be tidally locked, with one side always facing the star.
	\|-		\|-
	![[File:Star class b.jpg\|center\|thumb\|196x196px]]		![[File:Star class o.jpg\|center\|thumb\|196x196px]]
	\|O		\|O
	\|{{icon\|energy}}6-8		\|{{icon\|energy}}6-8
Line 46:		Line 46:
	\|A region of space where the gravitational pull is so strong that nothing, not even light, can escape. Black holes form when massive stars collapse in on themselves.		\|A region of space where the gravitational pull is so strong that nothing, not even light, can escape. Black holes form when massive stars collapse in on themselves.
	\|-		\|-
	![[File:Star ~~class b~~.jpg\|center\|thumb\|196x196px]]		![[File:Star pulsar.jpg\|center\|thumb\|196x196px]]
	\|Pulsar		\|Pulsar
	\|{{Icon\|energy}}1-2{{icon\|science}}1-2		\|{{Icon\|energy}}1-2{{icon\|science}}1-2
Line 61:		Line 61:
	\|The remnant core of a low-mass star that has exhausted all of its nuclear fuel. White dwarfs are small and dense, with a mass similar to the Sun but a size comparable to Earth. They emit little energy and eventually cool to become a "black dwarf."		\|The remnant core of a low-mass star that has exhausted all of its nuclear fuel. White dwarfs are small and dense, with a mass similar to the Sun but a size comparable to Earth. They emit little energy and eventually cool to become a "black dwarf."
	\|-		\|-
	![[File:Star ~~class b~~.jpg\|center\|thumb\|196x196px]]		![[File:Star supermassive black hole.jpg\|center\|thumb\|196x196px]]
	\|Supermassive Black Hole		\|Supermassive Black Hole
	\|{{Icon\|power}}5{{Icon\|science}}5-10		\|{{Icon\|power}}5{{Icon\|science}}5-10
	\|A supermassive black hole, residing at the center of galaxies, exerts an irresistible gravitational force, ensnaring even light within its inescapable grasp. Seizing control of the supermassive black hole at the heart of the galaxy bestows unparalleled dominion to the star empire, wielding influence over the cosmic fabric and commanding strategic advantages that can tip the balance of power in their favour.		\|A supermassive black hole, residing at the center of galaxies, exerts an irresistible gravitational force, ensnaring even light within its inescapable grasp. Seizing control of the supermassive black hole at the heart of the galaxy bestows unparalleled dominion to the star empire, wielding influence over the cosmic fabric and commanding strategic advantages that can tip the balance of power in their favour.
	\|}		\|}

ADAMJR at 01:03, 19 July 2024

2024-07-19T01:03:12Z

← Older revision		Revision as of 02:03, 19 July 2024
Line 1:		Line 1:
	Stars are the largest celestial bodies in the galaxy, and form the center of a star system where [[Planet\|planets]] orbit around.		Stars are the largest celestial bodies in the galaxy, and form the center of a star system where [[Planet\|planets]] orbit around.
	{\| class="wikitable"		{\| class="wikitable"
	\|+
	!		!
	!Type		!Type
Line 7:		Line 6:
	!Description		!Description
	\|-		\|-
	\|		![[File:Star class a.jpg\|center\|thumb\|196x196px]]
	\|A		\|A
	\|{{icon\|energy}}1-3		\|{{icon\|energy}}1-3
	\|A white star that is hotter and brighter than the Sun. It has a shorter lifespan than the Sun and emits ultraviolet radiation that can be harmful to life on nearby planets.		\|A white star that is hotter and brighter than the Sun. It has a shorter lifespan than the Sun and emits ultraviolet radiation that can be harmful to life on nearby planets.
	\|-		\|-
	\|		![[File:Star class b.jpg\|center\|thumb\|196x196px]]
	\|B		\|B
	\|{{icon\|energy}}2-3		\|{{icon\|energy}}2-3
	\|A blue star that burns very hot and bright, but has a relatively short lifespan. It emits high-energy radiation that can be harmful to nearby planets and spacecraft.		\|A blue star that burns very hot and bright, but has a relatively short lifespan. It emits high-energy radiation that can be harmful to nearby planets and spacecraft.
	\|-		\|-
	\|		![[File:Star class b.jpg\|center\|thumb\|196x196px]]
	\|F		\|F
	\|{{icon\|energy}}1-2		\|{{icon\|energy}}1-2
	\|A yellow-white star that is slightly hotter and brighter than the Sun. It has a longer lifespan and is more stable than the Sun.		\|A yellow-white star that is slightly hotter and brighter than the Sun. It has a longer lifespan and is more stable than the Sun.
	\|-		\|-
	\|		![[File:Star class b.jpg\|center\|thumb\|196x196px]]
	\|G		\|G
	\|{{icon\|energy}}1-2		\|{{icon\|energy}}1-2
	\|A yellow star like our Sun. It is relatively stable and has a long lifespan, making it a good candidate for hosting habitable planets.		\|A yellow star like our Sun. It is relatively stable and has a long lifespan, making it a good candidate for hosting habitable planets.
	\|-		\|-
	\|		![[File:Star class b.jpg\|center\|thumb\|196x196px]]
	\|K		\|K
	\|{{icon\|energy}}1		\|{{icon\|energy}}1
	\|An orange star that is cooler and less luminous than the Sun. It has a long lifespan but emits less energy than the Sun, which can make it difficult for planets to maintain a habitable temperature.		\|An orange star that is cooler and less luminous than the Sun. It has a long lifespan but emits less energy than the Sun, which can make it difficult for planets to maintain a habitable temperature.
	\|-		\|-
	\|		![[File:Star class b.jpg\|center\|thumb\|196x196px]]
	\|M		\|M
	\|{{icon\|energy}}1		\|{{icon\|energy}}1
	\|A red star that is the most common type of star in the galaxy. It is relatively cool and dim, with a long lifespan. Planets in the habitable zone of a Class-M star would be close to the star and would likely be tidally locked, with one side always facing the star.		\|A red star that is the most common type of star in the galaxy. It is relatively cool and dim, with a long lifespan. Planets in the habitable zone of a Class-M star would be close to the star and would likely be tidally locked, with one side always facing the star.
	\|-		\|-
	\|		![[File:Star class b.jpg\|center\|thumb\|196x196px]]
	\|O		\|O
	\|{{icon\|energy}}6-8		\|{{icon\|energy}}6-8
	\|A rare and very hot blue star that is much larger and more massive than the Sun. It emits intense ultraviolet radiation and has a short lifespan.		\|A rare and very hot blue star that is much larger and more massive than the Sun. It emits intense ultraviolet radiation and has a short lifespan.
	\|-		\|-
	\|		![[File:Star black hole.jpg\|center\|thumb\|196x196px]]
	\|Black Hole		\|Black Hole
	\|{{icon\|science}}2-4		\|{{icon\|science}}2-4
	\|A region of space where the gravitational pull is so strong that nothing, not even light, can escape. Black holes form when massive stars collapse in on themselves.		\|A region of space where the gravitational pull is so strong that nothing, not even light, can escape. Black holes form when massive stars collapse in on themselves.
	\|-		\|-
	\|		![[File:Star class b.jpg\|center\|thumb\|196x196px]]
	\|Pulsar		\|Pulsar
	\|{{Icon\|energy}}1-2{{icon\|science}}1-2		\|{{Icon\|energy}}1-2{{icon\|science}}1-2
	\|A highly magnetized, rotating neutron star that emits beams of electromagnetic radiation. Pulsars were first observed as objects emitting regular pulses of radio waves.		\|A highly magnetized, rotating neutron star that emits beams of electromagnetic radiation. Pulsars were first observed as objects emitting regular pulses of radio waves.
	\|-		\|-
	\|		![[File:Star neutron.jpg\|center\|thumb\|196x196px]]
	\|Neutron Star		\|Neutron Star
	\|{{Icon\|energy}}1-2{{icon\|science}}1-2		\|{{Icon\|energy}}1-2{{icon\|science}}1-2
	\|The collapsed core of a massive star that has gone supernova. Neutron stars are incredibly dense, with a mass greater than the Sun packed into a sphere just a few kilometers in diameter.		\|The collapsed core of a massive star that has gone supernova. Neutron stars are incredibly dense, with a mass greater than the Sun packed into a sphere just a few kilometers in diameter.
	\|-		\|-
	\|		![[File:Star white dwarf.jpg\|center\|thumb\|196x196px]]
	\|White Dwarf		\|White Dwarf
	\|{{Icon\|power}}1		\|{{Icon\|power}}1
	\|The remnant core of a low-mass star that has exhausted all of its nuclear fuel. White dwarfs are small and dense, with a mass similar to the Sun but a size comparable to Earth. They emit little energy and eventually cool to become a "black dwarf."		\|The remnant core of a low-mass star that has exhausted all of its nuclear fuel. White dwarfs are small and dense, with a mass similar to the Sun but a size comparable to Earth. They emit little energy and eventually cool to become a "black dwarf."
	\|-		\|-
	\|		![[File:Star class b.jpg\|center\|thumb\|196x196px]]
	\|Supermassive Black Hole		\|Supermassive Black Hole
	\|{{Icon\|power}}5{{Icon\|science}}5-10		\|{{Icon\|power}}5{{Icon\|science}}5-10
	\|A supermassive black hole, residing at the center of galaxies, exerts an irresistible gravitational force, ensnaring even light within its inescapable grasp. Seizing control of the supermassive black hole at the heart of the galaxy bestows unparalleled dominion to the star empire, wielding influence over the cosmic fabric and commanding strategic advantages that can tip the balance of power in their favour.		\|A supermassive black hole, residing at the center of galaxies, exerts an irresistible gravitational force, ensnaring even light within its inescapable grasp. Seizing control of the supermassive black hole at the heart of the galaxy bestows unparalleled dominion to the star empire, wielding influence over the cosmic fabric and commanding strategic advantages that can tip the balance of power in their favour.
	\|}		\|}

ADAMJR: Add resources to stars table

2024-07-18T20:35:08Z

Add resources to stars table

← Older revision		Revision as of 21:35, 18 July 2024
Line 9:		Line 9:
	\|		\|
	\|A		\|A
	\|		\|{{icon\|energy}}1-3
	\|A white star that is hotter and brighter than the Sun. It has a shorter lifespan than the Sun and emits ultraviolet radiation that can be harmful to life on nearby planets.		\|A white star that is hotter and brighter than the Sun. It has a shorter lifespan than the Sun and emits ultraviolet radiation that can be harmful to life on nearby planets.
	\|-		\|-
	\|		\|
	\|B		\|B
	\|		\|{{icon\|energy}}2-3
	\|A blue star that burns very hot and bright, but has a relatively short lifespan. It emits high-energy radiation that can be harmful to nearby planets and spacecraft.		\|A blue star that burns very hot and bright, but has a relatively short lifespan. It emits high-energy radiation that can be harmful to nearby planets and spacecraft.
	\|-		\|-
	\|		\|
	\|F		\|F
	\|		\|{{icon\|energy}}1-2
	\|A yellow-white star that is slightly hotter and brighter than the Sun. It has a longer lifespan and is more stable than the Sun.		\|A yellow-white star that is slightly hotter and brighter than the Sun. It has a longer lifespan and is more stable than the Sun.
	\|-		\|-
	\|		\|
	\|G		\|G
	\|		\|{{icon\|energy}}1-2
	\|A yellow star like our Sun. It is relatively stable and has a long lifespan, making it a good candidate for hosting habitable planets.		\|A yellow star like our Sun. It is relatively stable and has a long lifespan, making it a good candidate for hosting habitable planets.
	\|-		\|-
	\|		\|
	\|K		\|K
	\|		\|{{icon\|energy}}1
	\|An orange star that is cooler and less luminous than the Sun. It has a long lifespan but emits less energy than the Sun, which can make it difficult for planets to maintain a habitable temperature.		\|An orange star that is cooler and less luminous than the Sun. It has a long lifespan but emits less energy than the Sun, which can make it difficult for planets to maintain a habitable temperature.
	\|-		\|-
	\|		\|
	\|M		\|M
	\|		\|{{icon\|energy}}1
	\|A red star that is the most common type of star in the galaxy. It is relatively cool and dim, with a long lifespan. Planets in the habitable zone of a Class-M star would be close to the star and would likely be tidally locked, with one side always facing the star.		\|A red star that is the most common type of star in the galaxy. It is relatively cool and dim, with a long lifespan. Planets in the habitable zone of a Class-M star would be close to the star and would likely be tidally locked, with one side always facing the star.
	\|-		\|-
	\|		\|
	\|O		\|O
	\|		\|{{icon\|energy}}6-8
	\|A rare and very hot blue star that is much larger and more massive than the Sun. It emits intense ultraviolet radiation and has a short lifespan.		\|A rare and very hot blue star that is much larger and more massive than the Sun. It emits intense ultraviolet radiation and has a short lifespan.
	\|-		\|-
	\|		\|
	\|Black Hole		\|Black Hole
	\|		\|{{icon\|science}}2-4
	\|A region of space where the gravitational pull is so strong that nothing, not even light, can escape. Black holes form when massive stars collapse in on themselves.		\|A region of space where the gravitational pull is so strong that nothing, not even light, can escape. Black holes form when massive stars collapse in on themselves.
	\|-		\|-
	\|		\|
	\|Pulsar		\|Pulsar
	\|		\|{{Icon\|energy}}1-2{{icon\|science}}1-2
	\|A highly magnetized, rotating neutron star that emits beams of electromagnetic radiation. Pulsars were first observed as objects emitting regular pulses of radio waves.		\|A highly magnetized, rotating neutron star that emits beams of electromagnetic radiation. Pulsars were first observed as objects emitting regular pulses of radio waves.
	\|-		\|-
	\|		\|
	\|Neutron Star		\|Neutron Star
	\|		\|{{Icon\|energy}}1-2{{icon\|science}}1-2
	\|The collapsed core of a massive star that has gone supernova. Neutron stars are incredibly dense, with a mass greater than the Sun packed into a sphere just a few kilometers in diameter.		\|The collapsed core of a massive star that has gone supernova. Neutron stars are incredibly dense, with a mass greater than the Sun packed into a sphere just a few kilometers in diameter.
	\|-		\|-
	\|		\|
	\|White Dwarf		\|White Dwarf
	\|		\|{{Icon\|power}}1
	\|The remnant core of a low-mass star that has exhausted all of its nuclear fuel. White dwarfs are small and dense, with a mass similar to the Sun but a size comparable to Earth. They emit little energy and eventually cool to become a "black dwarf."		\|The remnant core of a low-mass star that has exhausted all of its nuclear fuel. White dwarfs are small and dense, with a mass similar to the Sun but a size comparable to Earth. They emit little energy and eventually cool to become a "black dwarf."
	\|-		\|-
	\|		\|
	\|Supermassive Black Hole		\|Supermassive Black Hole
	\|		\|{{Icon\|power}}5{{Icon\|science}}5-10
	\|A supermassive black hole, residing at the center of galaxies, exerts an irresistible gravitational force, ensnaring even light within its inescapable grasp. Seizing control of the supermassive black hole at the heart of the galaxy bestows unparalleled dominion to the star empire, wielding influence over the cosmic fabric and commanding strategic advantages that can tip the balance of power in their favour.		\|A supermassive black hole, residing at the center of galaxies, exerts an irresistible gravitational force, ensnaring even light within its inescapable grasp. Seizing control of the supermassive black hole at the heart of the galaxy bestows unparalleled dominion to the star empire, wielding influence over the cosmic fabric and commanding strategic advantages that can tip the balance of power in their favour.
	\|}		\|}

ADAMJR: Create page

2024-07-17T18:51:48Z

Create page

New page

Stars are the largest celestial bodies in the galaxy, and form the center of a star system where [[Planet|planets]] orbit around.
{| class="wikitable"
|+
!
!Type
!Resources
!Description
|-
|
|A
|
|A white star that is hotter and brighter than the Sun. It has a shorter lifespan than the Sun and emits ultraviolet radiation that can be harmful to life on nearby planets.
|-
|
|B
|
|A blue star that burns very hot and bright, but has a relatively short lifespan. It emits high-energy radiation that can be harmful to nearby planets and spacecraft.
|-
|
|F
|
|A yellow-white star that is slightly hotter and brighter than the Sun. It has a longer lifespan and is more stable than the Sun.
|-
|
|G
|
|A yellow star like our Sun. It is relatively stable and has a long lifespan, making it a good candidate for hosting habitable planets.
|-
|
|K
|
|An orange star that is cooler and less luminous than the Sun. It has a long lifespan but emits less energy than the Sun, which can make it difficult for planets to maintain a habitable temperature.
|-
|
|M
|
|A red star that is the most common type of star in the galaxy. It is relatively cool and dim, with a long lifespan. Planets in the habitable zone of a Class-M star would be close to the star and would likely be tidally locked, with one side always facing the star.
|-
|
|O
|
|A rare and very hot blue star that is much larger and more massive than the Sun. It emits intense ultraviolet radiation and has a short lifespan.
|-
|
|Black Hole
|
|A region of space where the gravitational pull is so strong that nothing, not even light, can escape. Black holes form when massive stars collapse in on themselves.
|-
|
|Pulsar
|
|A highly magnetized, rotating neutron star that emits beams of electromagnetic radiation. Pulsars were first observed as objects emitting regular pulses of radio waves.
|-
|
|Neutron Star
|
|The collapsed core of a massive star that has gone supernova. Neutron stars are incredibly dense, with a mass greater than the Sun packed into a sphere just a few kilometers in diameter.
|-
|
|White Dwarf
|
|The remnant core of a low-mass star that has exhausted all of its nuclear fuel. White dwarfs are small and dense, with a mass similar to the Sun but a size comparable to Earth. They emit little energy and eventually cool to become a "black dwarf."
|-
|
|Supermassive Black Hole
|
|A supermassive black hole, residing at the center of galaxies, exerts an irresistible gravitational force, ensnaring even light within its inescapable grasp. Seizing control of the supermassive black hole at the heart of the galaxy bestows unparalleled dominion to the star empire, wielding influence over the cosmic fabric and commanding strategic advantages that can tip the balance of power in their favour.
|}