Star Motion on the Horizon JS Package

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Star Motion on the Horizon JS Package

written by Mario Belloni and Kristen Thompson

The Star Motion on the Horizon JS Package displays how the appearance and motion of the stars near and around the northern, southern, eastern, and western horizon change over the course of hours. The specific latitude modeled can be changed with a slider. The north celestial pole (NCP) is shown in yellow and star trails are shown in white.

The Star Motion on the Horizon JS Package was developed using the Easy JavaScript Simulations (EjS) version 6. It is distributed as a ready-to-run html page and requires only a browser with JavaScript support. This model runs on tablets.

.zip

Star Motion on the Horizon JS Package

download 835kb .zip
Published: July 26, 2019
previous versions

Star Motion on the Horizon JS Package ePub
The ePub version of the Star Motion on the Horizon JS Package.
download 327kb .epub
Published: July 25, 2019
Released under a CC Noncommercial-Share Alike license.

4 ready-to-run examples are available

1 ready-to-edit examples are available

Open Star Motion on the Horizon JS Package Source Code in Web EJS

1 source code document is available

.zip

Star Motion on the Horizon JS Package Source Code
Source code for the Star Motion on the Horizon JS Package.
download 29kb .zip
Published: July 25, 2019
Released under a CC Noncommercial-Share Alike license.
previous versions

Subjects	Levels	Resource Types
Astronomy - Fundamentals = Night Sky	- High School - Lower Undergraduate - Middle School	- Instructional Material = Interactive Simulation - Audio/Visual = Image/Image Set

Intended Users	Formats	Ratings
- Learners - Educators - General Publics	- application/javascript	Currently 0.0/5 Want to rate this material? Login here!

Access Rights:: Free access
License:: This material is released under a Creative Commons Attribution-Noncommercial-Share Alike 3.0 license.
Rights Holder:: Mario Belloni
Merlot:: pending
Keywords:: EJS, EJSS, Easy Java Simulations, JavaScript, OSP, Open Source Physics, astronomy simulation, east, horizon, north, rising, setting, south, star motion, west
Record Cloner:: Metadata instance created July 26, 2019 by Mario Belloni
Record Updated:: October 29, 2021 by Lyle Barbato
Last Update when Cataloged:: July 26, 2019
Other Collections:: The Astronomy Center

The Open Source Physics

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AAAS Benchmark Alignments (2008 Version)

4. The Physical Setting

4A. The Universe

K-2: 4A/P2. The sun can be seen only in the daytime, but the moon can be seen sometimes at night and sometimes during the day. The sun, moon, and stars all appear to move slowly across the sky.
K-2: 4A/P3. The moon looks a little different every day but looks the same again about every four weeks.

4B. The Earth

6-8: 4B/M5. The moon's orbit around the earth once in about 28 days changes what part of the moon is lighted by the sun and how much of that part can be seen from the earth- the phases of the moon.

11. Common Themes

11B. Models

6-8: 11B/M1. Models are often used to think about processes that happen too slowly, too quickly, or on too small a scale to observe directly. They are also used for processes that are too vast, too complex, or too dangerous to study.

NSES Content Standards

Con.D: Earth & Space Science

K-4: Objects in the Sky
K-4: Changes in Earth & Sky

NSES Professional Development Standards

PD.A: Learn Science Content through Inquiry

Active Investigation: Involve teachers in actively investigating phenomena that can be studied scientifically, interpreting results, and making sense of findings consistent with currently accepted scientific understanding.

ComPADRE is beta testing Citation Styles!

Record Link

<a href="https://psrc.aapt.org/items/detail.cfm?ID=15117">Belloni, Mario, and Kristen Thompson. "Star Motion on the Horizon JS Package." Version 1.0.</a>

AIP Format

M. Belloni and K. Thompson, Computer Program STAR MOTION ON THE HORIZON JS PACKAGE, Version 1.0 (2019), WWW Document, (https://www.compadre.org/Repository/document/ServeFile.cfm?ID=15117&DocID=5082).

AJP/PRST-PER

M. Belloni and K. Thompson, Computer Program STAR MOTION ON THE HORIZON JS PACKAGE, Version 1.0 (2019), <https://www.compadre.org/Repository/document/ServeFile.cfm?ID=15117&DocID=5082>.

APA Format

Belloni, M., & Thompson, K. (2019). Star Motion on the Horizon JS Package (Version 1.0) [Computer software]. Retrieved December 11, 2024, from https://www.compadre.org/Repository/document/ServeFile.cfm?ID=15117&DocID=5082

Chicago Format

Belloni, Mario, and Kristen Thompson. "Star Motion on the Horizon JS Package." Version 1.0. https://www.compadre.org/Repository/document/ServeFile.cfm?ID=15117&DocID=5082 (accessed 11 December 2024).

MLA Format

Belloni, Mario, and Kristen Thompson. Star Motion on the Horizon JS Package. Vers. 1.0. Computer software. 2019. 11 Dec. 2024 <https://www.compadre.org/Repository/document/ServeFile.cfm?ID=15117&DocID=5082>.

BibTeX Export Format

@misc{ Author = "Mario Belloni and Kristen Thompson", Title = {Star Motion on the Horizon JS Package}, Month = {July}, Year = {2019} }

Refer Export Format

%A Mario Belloni %A Kristen Thompson %T Star Motion on the Horizon JS Package %D July 26, 2019 %U https://www.compadre.org/Repository/document/ServeFile.cfm?ID=15117&DocID=5082 %O 1.0 %O application/javascript

EndNote Export Format

%0 Computer Program %A Belloni, Mario %A Thompson, Kristen %D July 26, 2019 %T Star Motion on the Horizon JS Package %7 1.0 %8 July 26, 2019 %U https://www.compadre.org/Repository/document/ServeFile.cfm?ID=15117&DocID=5082

Disclaimer: ComPADRE offers citation styles as a guide only. We cannot offer interpretations about citations as this is an automated procedure. Please refer to the style manuals in the Citation Source Information area for clarifications.

Citation Source Information

The AIP Style presented is based on information from the AIP Style Manual.

The APA Style presented is based on information from APA Style.org: Electronic References.

The Chicago Style presented is based on information from Examples of Chicago-Style Documentation.

The MLA Style presented is based on information from the MLA FAQ.

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