MS-ESS1-2 - Revision history

Conradrichman at 00:51, 12 May 2025

2025-05-12T00:51:55Z

Conradrichman at 11:12, 11 May 2025

2025-05-11T11:12:39Z

Conradrichman at 01:58, 11 May 2025

2025-05-11T01:58:37Z

Shirleyshameen at 13:29, 9 May 2025

2025-05-09T13:29:38Z

Carolineleonard at 15:42, 5 May 2025

2025-05-05T15:42:31Z

Carolineleonard at 17:59, 30 April 2025

2025-04-30T17:59:34Z

Conradrichman at 17:22, 11 April 2025

2025-04-11T17:22:52Z

Conrad: Created page with "{{learningstandard | ls = Develop and use a model to describe the role of gravity in the motions within galaxies and the solar system. | cs = Emphasis for the model is on grav..."

2023-07-29T23:54:27Z

Created page with "{{learningstandard | ls = Develop and use a model to describe the role of gravity in the motions within galaxies and the solar system. | cs = Emphasis for the model is on grav..."

New page

{{learningstandard
| ls = Develop and use a model to describe the role of gravity in the motions within galaxies and the solar system.
| cs = Emphasis for the model is on gravity as the force that holds together the solar system and Milky Way galaxy and controls orbital motions within them. Examples of models could include physical models (such as a model of the solar system scaled using various measures or computer visualizations of elliptical orbits) or conceptual models (such as mathematical proportions relative to the size of familiar objects such as students’ school or state).
| ab = Assessment does not include Kepler’s Laws of orbital motion or the apparent retrograde motion of the planets as viewed from Earth.
}}

== {{Resourcesheading}} ==
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== {{Assessmentheading}} ==
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== {{Dimensionsheading}} ==
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{{Dimensionstable
| SEP1 =
| DCI1 =
| CC1 =
}}

== {{Connectionsheading}} ==
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| LANG1 =
| MATH1 =
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{{Bottomnav
| SUBJECT = [[P-8]]
| TOPIC = MS. Space Systems
}}

@@ Line 6: / Line 6: @@
 }}
-{{PerformanceLevel}}
+{{PerformanceLevelMS}}
 {{PLTable
 | Level4 = Develop and use a model to describe the role of gravity, both qualitatively and quantitatively, in the formation and motions within galaxies and the solar system.
@@ Line 39: / Line 39: @@
 * Models can be used to represent systems and their interactions—such as inputs, processes and outputs—and energy and matter flows within systems.
 }}
+<!--
 == {{Connectionsheading}} ==
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 | MATH1 =
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+-->
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-{{DISPLAYTITLE:MS-ESS1-2 {{!}} Gravity}}
+{{DISPLAYTITLE:MS-ESS1-2 {{!}} Gravity and Orbits}}
 {{Navlinks|MS-ESS1-1|MS-ESS1-3|← MS-ESS1-1|MS-ESS1-3 →}}{{learningstandard
 | ls = Develop and use a model to describe the role of gravity in the motions within galaxies and the solar system.

← Older revision		Revision as of 13:29, 9 May 2025
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		+	{{DISPLAYTITLE:MS-ESS1-2 {{!}} Gravity}}
	{{Navlinks\|MS-ESS1-1\|MS-ESS1-3\|← MS-ESS1-1\|MS-ESS1-3 →}}{{learningstandard		{{Navlinks\|MS-ESS1-1\|MS-ESS1-3\|← MS-ESS1-1\|MS-ESS1-3 →}}{{learningstandard
	\| ls = Develop and use a model to describe the role of gravity in the motions within galaxies and the solar system.		\| ls = Develop and use a model to describe the role of gravity in the motions within galaxies and the solar system.

← Older revision		Revision as of 17:22, 11 April 2025
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	\| TOPIC = MS. Space Systems		\| TOPIC = MS. Space Systems
	}}		}}
		+	<metadesc>NYS Standard MS-ESS1-2: Develop and use a model to describe the role of gravity in the motions within galaxies and the solar system.</metadesc>

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-{{expandthissection2}} <!-- Remove this after this section has been expanded upon -->
+* [[Questions:Gravitational Forces#q5|Gravitational Forces Q32]]
 == {{Dimensionsheading}} ==

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 {{Bottomnav
-| SUBJECT = [[P-8]]
+| SUBJECT = [[MS]]
 | TOPIC = MS. Space Systems
 }}
 <metadesc>NYS Standard MS-ESS1-2: Develop and use a model to describe the role of gravity in the motions within galaxies and the solar system.</metadesc>

@@ Line 1: / Line 1: @@
-{{learningstandard
+{{Navlinks|MS-ESS1-1|MS-ESS1-3|← MS-ESS1-1|MS-ESS1-3 →}}{{learningstandard
 | ls = Develop and use a model to describe the role of gravity in the motions within galaxies and the solar system.
 | cs = Emphasis for the model is on gravity as the force that holds together the solar system and Milky Way galaxy and controls orbital motions within them. Examples of models could include physical models (such as a model of the solar system scaled using various measures or computer visualizations of elliptical orbits) or conceptual models (such as mathematical proportions relative to the size of familiar objects such as students’ school or state).
 | ab = Assessment does not include Kepler’s Laws of orbital motion or the apparent retrograde motion of the planets as viewed from Earth.
 }}
@@ Line 19: / Line 27: @@
 {{Dimensionstable
-| SEP1 =
+| SEP1 = Developing and Using Models
-| DCI1 =
+* Develop and use a model to describe phenomena.
-| CC1 =
+| DCI1 = ESS1.A: The Universe and Its Stars
 }}