Difference between revisions of "HS-ESS1-1"
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| + | {{DISPLAYTITLE:HS-ESS1-1 {{!}} The Sun and Its Energy}} | ||
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| + | ||HS-ESS1-2||HS-ESS1-2 → | ||
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{{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 | ||
the Sun’s core to release energy that eventually reaches Earth in the form of radiation. | 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. | | 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 = | + | | ab = Assessment does not include details of the atomic and sub-atomic processes involved with the Sun’s nuclear fusion. |
| + | }} | ||
| + | {{NYSEDspecific}} | ||
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| + | {{PerformanceLevel}} | ||
| + | {{PLTable | ||
| + | | Level5 = Develop and critique models, based on evidence, that illustrate the lifespan of the Sun, the role of nuclear fusion, and how energy from the Sun reaches Earth in the form of electromagnetic radiation, using scale, proportion, and quantity to evaluate the models’ validity and limitations in order to revise them. | ||
| + | | 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 <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 <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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| − | | SEP1 = | + | | SEP1 = Developing and Using Models |
| − | | DCI1 = | + | * Develop a model based on evidence to illustrate the relationships between systems or between components of a system. |
| − | | CC1 = | + | | 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 = 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. (secondary to HS-ESS1-1) | ||
| + | | CC1 = Scale, Proportion, and Quantity | ||
| + | * The significance of a phenomenon is dependent on the scale, proportion, and quantity at which it occurs. | ||
}} | }} | ||
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| MATH1 = | | MATH1 = | ||
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{{Pagecontributors}} | {{Pagecontributors}} | ||
{{Bottomnav | {{Bottomnav | ||
| − | | SUBJECT = [[Earth and Space Science]] | + | | SUBJECT = [[Earth and Space Science|{{#fas:earth-americas}} Earth and Space Science]] |
| 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> | ||
Latest revision as of 10:26, 10 May 2025
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.
Clarification statement: 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.
Assessment boundary: Assessment does not include details of the atomic and sub-atomic processes involved with the Sun’s nuclear fusion.
Note: this is a NYSED-specific performance expectation that is different from the Next Generation Science Standards.
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 five levels.
Develop and critique models, based on evidence, that illustrate the lifespan of the Sun, the role of nuclear fusion, and how energy from the Sun reaches Earth in the form of electromagnetic radiation, using scale, proportion, and quantity to evaluate the models’ validity and limitations in order to revise them.
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.
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).
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.
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.
Resources
Examples and discussion of resources for the learning, teaching, and assessment of HS-ESS1-1.
This section could be expanded upon. You can help out by adding to this section.
Assessment
What assessment of HS-ESS1-1 might look like on a NY state exam.
This section could be expanded upon. You can help out by adding to this section.
NGSS Dimensions
Performance expectation HS-ESS1-1 was developed using the following elements from the NRC document A Framework for K-12 Science Education:
Science and Engineering Practices
- Developing and Using Models
- Develop a model based on evidence to illustrate the relationships between systems or between components of a system.
Disciplinary Core Ideas
- 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.
- 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. (secondary to HS-ESS1-1)
Crosscutting Concepts
- Scale, Proportion, and Quantity
- The significance of a phenomenon is dependent on the scale, proportion, and quantity at which it occurs.
Page contributors: Caroline Leonard, Conrad Richman