Probing the First Stars & Galaxies : Show Me Science
(eVideo)
Contributors
Published
[Place of publication not identified] : TMW Media Group,, [2013].
Status
Description
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Format
eVideo
Language
English
Notes
General Note
Originally released by TMW Media Group, 2013.
General Note
Streaming video file encoded with permission for digital streaming by Infobase on February 08, 2017.
Restrictions on Access
Access requires authentication through Classroom Video On Demand.
Description
Visible light, which can be seen with our eyes, comprises a small sliver of the electromagnetic spectrum. The rest of the spectrum, from short wavelength gamma rays to long-wavelength radio waves, requires special instruments to detect. ALMA uses and array of radio telescopes to detect and study radio waves from space. Radio telescopes are typically large parabolic dish antennas used singly or in an array. Radio observatories are preferentially located far from major centers of population to avoid electromagnetic interference (EMI) from radio, TV, radar, and other EMI emitting devices. This is similar to the locating of optical telescopes to avoid light pollution, with the difference being that radio observatories are often placed in valleys to further shield them from EMI as opposed to clear air mountain tops for optical observatories. ALMA is an advanced tool for studying very old stars and galaxies. These objects now are seen at great cosmic distances, with most of their light stretched out to millimeter and sub-millimeter wavelengths by the expansion of the universe. ALMA provides the unprecedented ability to study the processes of star and planet formation. Unimpeded by the dust that obscures visible-light observations, ALMA will be able to reveal the details of young, still-forming stars, and is expected to show young planets still in the process of developing. In addition, ALMA will allow scientists to learn in detail about the complex chemistry of the giant clouds of gas and dust that spawn stars and planetary systems.
Target Audience
6 - 8, 9 - 12
System Details
Streaming video file.
System Details
System requirements: Classroom Video On Demand playback platform.
Citations
APA Citation, 7th Edition (style guide)
(2013). Probing the First Stars & Galaxies: Show Me Science . TMW Media Group, .
Chicago / Turabian - Author Date Citation, 17th Edition (style guide)2013. Probing the First Stars & Galaxies: Show Me Science. TMW Media Group.
Chicago / Turabian - Humanities (Notes and Bibliography) Citation, 17th Edition (style guide)Probing the First Stars & Galaxies: Show Me Science TMW Media Group, 2013.
MLA Citation, 9th Edition (style guide)Probing the First Stars & Galaxies: Show Me Science TMW Media Group, , 2013.
Note! Citations contain only title, author, edition, publisher, and year published. Citations should be used as a guideline and should be double checked for accuracy. Citation formats are based on standards as of August 2021.
Staff View
Grouped Work ID
c446caf1-3c58-13b2-9412-48154683ad8c-eng
Grouping Information
Grouped Work ID | c446caf1-3c58-13b2-9412-48154683ad8c-eng |
---|---|
Full title | probing the first stars and galaxies show me science |
Author | infobase |
Grouping Category | movie |
Last Update | 2023-01-17 14:42:32PM |
Last Indexed | 2024-04-19 00:40:31AM |
Book Cover Information
Image Source | classroomVideoOnDemand |
---|---|
First Loaded | Aug 15, 2022 |
Last Used | Jan 26, 2024 |
Marc Record
First Detected | Jul 23, 2018 12:00:00 AM |
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Last File Modification Time | Jan 17, 2023 02:43:23 PM |
MARC Record
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500 | |a Originally released by TMW Media Group, 2013. | ||
500 | |a Streaming video file encoded with permission for digital streaming by Infobase on February 08, 2017. | ||
505 | 0 | 0 | |t Advances in Astronomy (4:10); |t Examining TW Hydrae (3:23); |t ALMA Back End (2:11); |t Astrochemistry (3:13); |t Credits: Probing the First Stars and Galaxies: Show Me Science (0:13); |
506 | 1 | |a Access requires authentication through Classroom Video On Demand. | |
520 | |a Visible light, which can be seen with our eyes, comprises a small sliver of the electromagnetic spectrum. The rest of the spectrum, from short wavelength gamma rays to long-wavelength radio waves, requires special instruments to detect. ALMA uses and array of radio telescopes to detect and study radio waves from space. Radio telescopes are typically large parabolic dish antennas used singly or in an array. Radio observatories are preferentially located far from major centers of population to avoid electromagnetic interference (EMI) from radio, TV, radar, and other EMI emitting devices. This is similar to the locating of optical telescopes to avoid light pollution, with the difference being that radio observatories are often placed in valleys to further shield them from EMI as opposed to clear air mountain tops for optical observatories. ALMA is an advanced tool for studying very old stars and galaxies. These objects now are seen at great cosmic distances, with most of their light stretched out to millimeter and sub-millimeter wavelengths by the expansion of the universe. ALMA provides the unprecedented ability to study the processes of star and planet formation. Unimpeded by the dust that obscures visible-light observations, ALMA will be able to reveal the details of young, still-forming stars, and is expected to show young planets still in the process of developing. In addition, ALMA will allow scientists to learn in detail about the complex chemistry of the giant clouds of gas and dust that spawn stars and planetary systems. | ||
521 | 2 | |a 6 - 8, 9 - 12 | |
538 | |a Streaming video file. | ||
538 | |a System requirements: Classroom Video On Demand playback platform. | ||
588 | |a Title from distributor's description | ||
650 | 0 | |a Physical sciences. | |
650 | 0 | |a Space. | |
650 | 0 | |a Stars. | |
650 | 0 | |a Astronomy. | |
650 | 0 | |a Galaxies. | |
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830 | 0 | |a Show Me Science. | |
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