Difference between revisions of "MS-ESS1-3"
(Reorder sections: Assessment, then Performance Level Descriptions, then Resources) |
|||
| (4 intermediate revisions by 2 users not shown) | |||
| Line 1: | Line 1: | ||
| + | {{DISPLAYTITLE:MS-ESS1-3 {{!}} Scale of the Solar System}} | ||
{{Navlinks|MS-ESS1-2|MS-ESS1-4|← MS-ESS1-2|MS-ESS1-4 →}}{{learningstandard | {{Navlinks|MS-ESS1-2|MS-ESS1-4|← MS-ESS1-2|MS-ESS1-4 →}}{{learningstandard | ||
| ls = Analyze and interpret data to determine scale properties of objects in the solar system. | | ls = Analyze and interpret data to determine scale properties of objects in the solar system. | ||
| Line 5: | Line 6: | ||
| ab = Assessment does not include recalling facts about properties of the planets and other solar system bodies. | | ab = Assessment does not include recalling facts about properties of the planets and other solar system bodies. | ||
}} | }} | ||
| − | {{ | + | |
| + | == {{Assessmentheading}} == | ||
| + | {{assessmentmessage}} | ||
| + | |||
| + | {| class="wikitable" style="width:100%; text-align:center" | ||
| + | ! style="padding: 0.5em 1.5em;" | Exam | ||
| + | ! style="padding: 0.5em 1.5em;" | Cluster | ||
| + | ! style="padding: 0.5em 1.5em;" | Question | ||
| + | |- | ||
| + | | rowspan="2" style="background-color:white;" | [[Spring 2026 Grade 8 Science Test|Spring 2026]] | ||
| + | | style="background-color:white;" | [[Questions:Scale Properties in Our Solar System|Scale Properties in Our Solar System]] | ||
| + | | style="background-color:white;" | [[Questions:Scale Properties in Our Solar System#q3|Question 51]] | ||
| + | |- | ||
| + | | style="background-color:white;" | [[Questions:Scale Properties in Our Solar System|Scale Properties in Our Solar System]] | ||
| + | | style="background-color:white;" | [[Questions:Scale Properties in Our Solar System#q4|Question 52]] | ||
| + | |- | ||
| + | | rowspan="2" style="background-color:white;" | [[Spring 2025 Grade 8 Science Test|Spring 2025]] | ||
| + | | style="background-color:white;" | [[Questions:Observing Jupiter|Observing Jupiter]] | ||
| + | | style="background-color:white;" | [[Questions:Observing Jupiter#q1|Question 14]] | ||
| + | |- | ||
| + | | style="background-color:white;" | [[Questions:Observing Jupiter|Observing Jupiter]] | ||
| + | | style="background-color:white;" | [[Questions:Observing Jupiter#q2|Question 15]] | ||
| + | |} | ||
| + | |||
| + | {{PerformanceLevelMS}} | ||
{{PLTable | {{PLTable | ||
| Level4 = Analyze and interpret multiple data sets to determine scale properties of objects, including surface features and inner layers, in the solar system. | | Level4 = Analyze and interpret multiple data sets to determine scale properties of objects, including surface features and inner layers, in the solar system. | ||
| Line 12: | Line 37: | ||
| Level1 = Use data to determine the relative sizes and/or relative distances in the Earth-Sun-Moon system. | | Level1 = Use data to determine the relative sizes and/or relative distances in the Earth-Sun-Moon system. | ||
}} | }} | ||
| + | |||
== {{Resourcesheading}} == | == {{Resourcesheading}} == | ||
{{resourcesmessage}} | {{resourcesmessage}} | ||
{{expandthissection}} <!-- Remove this after this section has been expanded upon --> | {{expandthissection}} <!-- Remove this after this section has been expanded upon --> | ||
| − | |||
| − | |||
| − | |||
| − | |||
| − | |||
== {{Dimensionsheading}} == | == {{Dimensionsheading}} == | ||
| Line 33: | Line 54: | ||
* Time, space, and energy phenomena can be observed at various scales using models to study systems that are too large or too small. | * Time, space, and energy phenomena can be observed at various scales using models to study systems that are too large or too small. | ||
}} | }} | ||
| − | + | <!-- | |
== {{Connectionsheading}} == | == {{Connectionsheading}} == | ||
{{connectionsmessage}} | {{connectionsmessage}} | ||
| Line 42: | Line 63: | ||
| MATH1 = | | MATH1 = | ||
}} | }} | ||
| − | + | --> | |
{{Pagecontributors}} | {{Pagecontributors}} | ||
Latest revision as of 22:37, 20 September 2026
Analyze and interpret data to determine scale properties of objects in the solar system.
Clarification statement: Emphasis is on the analysis of data from Earth-based instruments, space-based telescopes, and spacecraft to determine similarities and differences among solar system objects. Examples of scale properties could include the sizes of an object’s layers (such as crust and atmosphere), surface features (such as volcanoes), and orbital radius. Examples of data could include statistical information, drawings and photographs, and models.
Assessment boundary: Assessment does not include recalling facts about properties of the planets and other solar system bodies.
Assessment
What assessment of MS-ESS1-3 might look like on a NY state exam.
Performance Level Descriptions
PLDs communicate the knowledge and skills expected of students to demonstrate proficiency in each Learning Standard. NYS assessments classify student performance into one of four levels.
Resources
Examples and discussion of resources for the learning, teaching, and assessment of MS-ESS1-3.
NGSS Dimensions
Performance expectation MS-ESS1-3 was developed using the following elements from the NRC document A Framework for K-12 Science Education:
- Analyzing and Interpreting Data
- Analyze and interpret data to determine similarities and differences in findings.
- ESS1.B: Earth and the Solar System
- (NYSED) The solar system consists of the Sun and a collection of objects, including planets, their moons, comets, and asteroids that are held in orbit around the Sun by its gravitational pull on them.
- Scale, Proportion, and Quantity
- Time, space, and energy phenomena can be observed at various scales using models to study systems that are too large or too small.