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Star Stuff: An Exploratory Case Study of the Cosmos Television Franchise

LAUNCH OF EXPLORER 1 SATELLITE 1958 "THE BIG PICTURE" EPISODE 71512

This episode of the U.S. Army's TV program "The Big Picture" deals with the the first satellite of the United States Explorer 1, launched as part of its participation in the International Geophysical Year. The mission followed the first two satellites the previous year; the Soviet Union's Sputnik 1 and 2, beginning the Cold War Space Race between the two nations. Army General John Medaris headed the Army Ballistic Missile Agency, which oversaw both JPL and Wernher von Braun’s rocket team in Huntsville, Ala. JPL and the Army teamed up to launch Explorer 1. The Huntsville team provided the first-stage rocket, while JPL built the upper stages and the satellite that carried the science payload. Medaris played a pivotal role in advancing the development of Explorer 1. Explorer 1 was launched on January 31, 1958 at 22:48 Eastern Time (equal to February 1, 03:48 UTC) atop the first Juno booster from LC-26 at the Cape Canaveral Missile Annex, Florida. It was the first spacecraft to detect the Van Allen radiation belt, returning data until its batteries were exhausted after nearly four months. It remained in orbit until 1970, and has been followed by more than 90 scientific spacecraft in the Explorer series. Explorer 1 was given Satellite Catalog Number 4, and the Harvard designation 1958 Alpha 1, the forerunner to the modern International Designator. To the surprise of mission experts, Explorer 1 changed rotation axis after launch. The elongated body of the spacecraft had been designed to spin about its long (least-inertia) axis but refused to do so, and instead started precessing due to energy dissipation from flexible structural elements. Later it was understood that on general grounds, the body ends up in the spin state that minimizes the kinetic rotational energy for a fixed angular momentum (this being the maximal-inertia axis). This motivated the first further development of the Eulerian theory of rigid body dynamics after nearly 200 years—to address this kind of momentum-preserving energy dissipation. Sometimes the instrumentation would report the expected cosmic ray count (approximately 30 counts per second) but sometimes it would show a peculiar zero counts per second. The University of Iowa (under Van Allen) noted that all of the zero counts per second reports were from an altitude of 2,000+ km (1,250+ miles) over South America, while passes at 500 km (310 mi) would show the expected level of cosmic rays. Later, after Explorer 3, it was concluded that the original Geiger counter had been overwhelmed ("saturated") by strong radiation coming from a belt of charged particles trapped in space by the Earth's magnetic field. This belt of charged particles is now known as the Van Allen radiation belt. The discovery was considered to be one of the outstanding discoveries of the International Geophysical Year. The acoustic micrometeorite detector detected 145 impacts of cosmic dust in 78,750 seconds. This calculates to an average impact rate of 8.0×10−3 impacts m−2 s−1 over the twelve-day period (29 impacts per hour per square meter). This film is part of the Periscope Film LLC archive, one of the largest historic military, transportation, and aviation stock footage collections in the USA. Entirely film backed, this material is available for licensing in 24p HD and 2K. For more information visit http://www.PeriscopeFilm.com

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1. LAUNCH OF EXPLORER 1 SATELLITE 1958 "THE BIG PICTURE" EPISODE 71512 This episode of the U.S. Army's TV program "The Big Picture" deals with the the first satellite of the United States Explorer 1, launched as part of its participation in the International Geophysical Year. The mission followed the first two satellites the previous year; the Soviet Union's Sputnik 1 and 2, beginning the Cold War Space Race between the two nations. Army General John Medaris headed the Army Ballistic Missile Agency, which oversaw both JPL and Wernher von Braun’s rocket team in Huntsville, Ala. JPL and the Army teamed up to launch Explorer 1. The Huntsville team provided the first-stage rocket, while JPL built the upper stages and the satellite that carried the science payload. Medaris played a pivotal role in advancing the development of Explorer 1. Explorer 1 was launched on January 31, 1958 at 22:48 Eastern Time (equal to February 1, 03:48 UTC) atop the first Juno booster from LC-26 at the Cape Canaveral Missile Annex, Florida. It was the first spacecraft to detect the Van Allen radiation belt, returning data until its batteries were exhausted after nearly four months. It remained in orbit until 1970, and has been followed by more than 90 scientific spacecraft in the Explorer series. Explorer 1 was given Satellite Catalog Number 4, and the Harvard designation 1958 Alpha 1, the forerunner to the modern International Designator. To the surprise of mission experts, Explorer 1 changed rotation axis after launch. The elongated body of the spacecraft had been designed to spin about its long (least-inertia) axis but refused to do so, and instead started precessing due to energy dissipation from flexible structural elements. Later it was understood that on general grounds, the body ends up in the spin state that minimizes the kinetic rotational energy for a fixed angular momentum (this being the maximal-inertia axis). This motivated the first further development of the Eulerian theory of rigid body dynamics after nearly 200 years—to address this kind of momentum-preserving energy dissipation. Sometimes the instrumentation would report the expected cosmic ray count (approximately 30 counts per second) but sometimes it would show a peculiar zero counts per second. The University of Iowa (under Van Allen) noted that all of the zero counts per second reports were from an altitude of 2,000+ km (1,250+ miles) over South America, while passes at 500 km (310 mi) would show the expected level of cosmic rays. Later, after Explorer 3, it was concluded that the original Geiger counter had been overwhelmed ("saturated") by strong radiation coming from a belt of charged particles trapped in space by the Earth's magnetic field. This belt of charged particles is now known as the Van Allen radiation belt. The discovery was considered to be one of the outstanding discoveries of the International Geophysical Year. The acoustic micrometeorite detector detected 145 impacts of cosmic dust in 78,750 seconds. This calculates to an average impact rate of 8.0×10−3 impacts m−2 s−1 over the twelve-day period (29 impacts per hour per square meter). This film is part of the Periscope Film LLC archive, one of the largest historic military, transportation, and aviation stock footage collections in the USA. Entirely film backed, this material is available for licensing in 24p HD and 2K. For more information visit http://www.PeriscopeFilm.com

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1. LAUNCH OF EXPLORER 1 SATELLITE 1958 "THE BIG PICTURE" EPISODE 71512 This episode of the U.S. Army's TV program "The Big Picture" deals with the the first satellite of the United States Explorer 1, launched as part of its participation in the International Geophysical Year. The mission followed the first two satellites the previous year; the Soviet Union's Sputnik 1 and 2, beginning the Cold War Space Race between the two nations. Army General John Medaris headed the Army Ballistic Missile Agency, which oversaw both JPL and Wernher von Braun’s rocket team in Huntsville, Ala. JPL and the Army teamed up to launch Explorer 1. The Huntsville team provided the first-stage rocket, while JPL built the upper stages and the satellite that carried the science payload. Medaris played a pivotal role in advancing the development of Explorer 1. Explorer 1 was launched on January 31, 1958 at 22:48 Eastern Time (equal to February 1, 03:48 UTC) atop the first Juno booster from LC-26 at the Cape Canaveral Missile Annex, Florida. It was the first spacecraft to detect the Van Allen radiation belt, returning data until its batteries were exhausted after nearly four months. It remained in orbit until 1970, and has been followed by more than 90 scientific spacecraft in the Explorer series. Explorer 1 was given Satellite Catalog Number 4, and the Harvard designation 1958 Alpha 1, the forerunner to the modern International Designator. To the surprise of mission experts, Explorer 1 changed rotation axis after launch. The elongated body of the spacecraft had been designed to spin about its long (least-inertia) axis but refused to do so, and instead started precessing due to energy dissipation from flexible structural elements. Later it was understood that on general grounds, the body ends up in the spin state that minimizes the kinetic rotational energy for a fixed angular momentum (this being the maximal-inertia axis). This motivated the first further development of the Eulerian theory of rigid body dynamics after nearly 200 years—to address this kind of momentum-preserving energy dissipation. Sometimes the instrumentation would report the expected cosmic ray count (approximately 30 counts per second) but sometimes it would show a peculiar zero counts per second. The University of Iowa (under Van Allen) noted that all of the zero counts per second reports were from an altitude of 2,000+ km (1,250+ miles) over South America, while passes at 500 km (310 mi) would show the expected level of cosmic rays. Later, after Explorer 3, it was concluded that the original Geiger counter had been overwhelmed ("saturated") by strong radiation coming from a belt of charged particles trapped in space by the Earth's magnetic field. This belt of charged particles is now known as the Van Allen radiation belt. The discovery was considered to be one of the outstanding discoveries of the International Geophysical Year. The acoustic micrometeorite detector detected 145 impacts of cosmic dust in 78,750 seconds. This calculates to an average impact rate of 8.0×10−3 impacts m−2 s−1 over the twelve-day period (29 impacts per hour per square meter). This film is part of the Periscope Film LLC archive, one of the largest historic military, transportation, and aviation stock footage collections in the USA. Entirely film backed, this material is available for licensing in 24p HD and 2K. For more information visit http://www.PeriscopeFilm.com

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The Cold War Space Race You have just entered the Cold War space race section of this project. This section will briefly summarize some of the major moments in space exploration history from the 1950s and 60s that the Cosmos documentaries were in direct conversation with. The Cold War space race between the United States and the Soviet Union began while Carl Sagan was a graduate student, working to acquire his Ph.D. It started when the Soviet Union launched Sputnik 1, the first off-Earth satellite that went into orbit on October 4, 1957. The Soviet’s ability to spy on other countries or launch weapons from outer space worried the United States. They would successfully launch their own satellite in response on January 31, 1958. This satellite was called Explorer 1. The National Aeronautics and Space Administration, better known as NASA, was formed that summer on July 29, 1958. Below is a 17-minute clip from a documentary television series called The Big Picture, which documented the launch of Explorer 1 from its very inception. Feel free to watch as much of it as you like.

Carl Sagan’s early work as a young scientist was focused on unmanned space probes designed to study nearby planets without carrying human passengers. The Mariner 2 mission to Venus serves as a notable example of that. Here's a picture of a Mariner 2 model being delivered to then U.S. President John F. Kennedy. The probe would eventually launch on August 4, 1962.
One month after Mariner 2’s launch, President Kennedy would give his famous speech at Rice University stadium. In the speech, he challenged America’s scientists to send a man to the moon and safely return him to Earth before the end of the decade. If you would like a refresher on the objectives outlined in this speech, I have provided a 15-minute excerpt for you to watch below.

Though President Kennedy was assassinated on November 22, 1963, his goal of landing an American astronaut on the moon was achieved by the Apollo 11 mission on July 16, 1969. Here's a select 13-minute portion of a documentary titled flight of Apollo 11. The Eagle has landed. This documentary was released that same year to document the achievement. I have selected 13 minutes for you to view at your leisure.

Upon returning to Earth, the Apollo 11 crew addressed the United States Congress. The three speeches given by each member of the Apollo 11 Team highlight their vision for the future of the United States in outer space after the completion of their historic trip. All 14 minutes of these speeches are available for you to watch below. You can watch as much of it as you like. Once you are done, you can continue on to the section covering Sagan’s work on the Pioneer Viking and Voyager space probes by clicking the blue button at the bottom of the page. You can also return to the homepage or use the toolbar at the top of your screen to select whichever sections of the project you would like to view next.