HS-ESS1-1 - Revision history

Carolineleonard at 14:26, 10 May 2025

2025-05-10T14:26:35Z

Conradrichman at 18:41, 5 May 2025

2025-05-05T18:41:39Z

Conradrichman at 01:30, 29 April 2025

2025-04-29T01:30:29Z

Carolineleonard at 22:13, 15 April 2025

2025-04-15T22:13:25Z

Carolineleonard at 22:12, 15 April 2025

2025-04-15T22:12:23Z

Conradrichman at 13:26, 14 April 2025

2025-04-14T13:26:56Z

Conradrichman at 00:07, 11 April 2025

2025-04-11T00:07:30Z

Conradrichman at 11:20, 2 April 2025

2025-04-02T11:20:23Z

Conradrichman at 00:47, 1 April 2025

2025-04-01T00:47:01Z

Conradrichman at 00:46, 1 April 2025

2025-04-01T00:46:18Z

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 {{Dimensionstable
-| SEP1 = Developing and using models
+| SEP1 = Developing and Using Models
 * Develop a model based on evidence to illustrate the relationships between systems or between components of a system.
-| DCI1 = The universe and its stars
+| DCI1 = ESS1.A: The Universe and Its Stars
 * The star called the sun is changing and will burn out over a lifespan of approximately 10 billion years.
-| DCI2 = Energy in chemical processes and everyday life
+| DCI2 = PS3.D: Energy in Chemical Processes and Everyday Life
-* Nuclear Fusion processes in the center of the sun release the energy that ultimately reaches Earth as radiation.
+* Nuclear Fusion processes in the center of the sun release the energy that ultimately reaches Earth as radiation. (secondary to HS-ESS1-1)
-| CC1 = Scale, proportion, and quantity
+| CC1 = Scale, Proportion, and Quantity
 * The significance of a phenomenon is dependent on the scale, proportion, and quantity at which it occurs.
 }}

@@ Line 34: / Line 34: @@
 {{Dimensionstable
-| SEP1 = Developing and using models: Develop a model based on evidence to illustrate the relationships between systems or between components of a system.
+| SEP1 = Developing and using models
-| DCI1 = The universe and its stars: The star called the sun is changing and will burn out over a lifespan of approximately 10 billion years.
+* Develop a model based on evidence to illustrate the relationships between systems or between components of a system.
-| DCI2 = Energy in chemical processes and everyday life: Nuclear Fusion processes in the center of the sun release the energy that ultimately reaches Earth as radiation.
+| DCI1 = The universe and its stars
-| CC1 = Scale, proportion, and quantity: The significance of a phenomenon is dependent on the scale, proportion, and quantity at which it occurs.
+* The star called the sun is changing and will burn out over a lifespan of approximately 10 billion years.
 }}
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← Older revision		Revision as of 01:30, 29 April 2025
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		+	{{DISPLAYTITLE:HS-ESS1-1 {{!}} The Sun and Its Energy}}
	{{Navlinks		{{Navlinks
	\|\|HS-ESS1-2\|\|HS-ESS1-2 →		\|\|HS-ESS1-2\|\|HS-ESS1-2 →

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 | Level4 = Develop a model based on evidence to illustrate the lifespan of the Sun and the role of nuclear fusion in the Sun’s core to release energy that eventually reaches Earth in the form of radiation.
 | Level3 = Complete a model based on evidence to illustrate the lifespan of the Sun and/or the role of nuclear fusion in the Sun’s core to release energy that eventually reaches Earth (in the form of radiation).
-| Level2 = Given a model, and/or information, describe the evidence that determines the lifespan of the Sun or illustrates the role of nuclear fusion in the Sun’s core to release energy or ways that the Sun’s radiation varies.
+| Level2 = Given a model, and/or information, describe the evidence that determines the lifespan of the Sun <b><u>or</u></b> illustrates the role of nuclear fusion in the Sun’s core to release energy <b><u>or</u></b> ways that the Sun’s radiation varies.
-| Level1 = Given a model, and/or information, identify the evidence, from those provided, that determines the lifespan of the Sun or illustrates the role of nuclear fusion in the Sun’s core to release energy or identify the correct pattern, from those provided, that shows variation in solar output.
+| Level1 = Given a model, and/or information, identify the evidence, from those provided, that determines the lifespan of the Sun <b><u>or</u></b> illustrates the role of nuclear fusion in the Sun’s core to release energy <b><u>or</u></b> identify the correct pattern, from those provided, that shows variation in solar output.
 }}

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 }}
 {{NYSEDspecific}}
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← Older revision		Revision as of 13:26, 14 April 2025
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		+	{{Navlinks
		+	\|\|HS-ESS1-2\|\|HS-ESS1-2 →
		+	}}
	{{learningstandard		{{learningstandard
	\| ls = Develop a model based on evidence to illustrate the life span of the Sun and the role of nuclear fusion in		\| ls = Develop a model based on evidence to illustrate the life span of the Sun and the role of nuclear fusion in

← Older revision		Revision as of 00:07, 11 April 2025
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	\| TOPIC = HS. Space Systems		\| TOPIC = HS. Space Systems
	}}		}}
		+	<metadesc>NYS Standard HS-ESS1-1: Develop a model based on evidence to illustrate the life span of the Sun and the role of nuclear fusion in the Sun’s core to release energy that eventually reaches Earth in the form of radiation.</metadesc>

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 | CC1 =
 }}
+<!--
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 | MATH1 =
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+-->
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 the Sun’s core to release energy that eventually reaches Earth in the form of radiation.
 | cs = Emphasis is on the energy transfer mechanisms that allow energy from nuclear fusion in the Sun’s core to reach Earth. Examples of evidence for the model could include observations of the masses and lifetimes of other stars, as well as the ways that the Sun’s radiation varies due to sudden solar flares (“space weather”), the 11-year sunspot cycle, and non-cyclic variations over centuries.
-| ab = Emphasis is on the energy transfer mechanisms that allow energy from nuclear fusion in the Sun’s core to reach Earth. Examples of evidence for the model could include observations of the masses and lifetimes of other stars, as well as the ways that the Sun’s radiation varies due to sudden solar flares (“space weather”), the 11-year sunspot cycle, and non-cyclic variations over centuries.
+| ab = Assessment does not include details of the atomic and sub-atomic processes involved with the Sun’s nuclear fusion.
 }}
 {{NYSEDspecific}}