ArticleslgStudy

science

Galactic Radiation and Background

Galactic Radiation and Background is a science topic covered in the lgStudy science library. This page brings together a partial reference excerpt, illustrations, worked examples, real-world applications and a short study plan, so you can understand Galactic Radiation and Background rather than just read about it. In short: Galactic Radiation and Background (GRAB) was the first successful United States orbital surveillance program, comprising a series of five Naval Research Laboratory electronic surveillance and solar astronomy satellites, launched from 1960 to 1962. Though only two of the five satellites made it into orbit, they returned a wealth of information on Soviet air defense radar capabilities as well as useful astronomical ob…

Galactic Radiation and Background — main illustration
Galactic Radiation and Background — illustration

Key takeaways

  • Galactic Radiation and Background belongs to science; place it in that map before memorising details.
  • Learn the definition first, then one example that makes the definition concrete.
  • Connect Galactic Radiation and Background to a quantity you can measure, compute or draw — that is where exam questions come from.
  • Reproduce the core statement of Galactic Radiation and Background from memory before moving on to harder problems.

Reference excerpt

Galactic Radiation and Background (GRAB) was the first successful United States orbital surveillance program, comprising a series of five Naval Research Laboratory electronic surveillance and solar astronomy satellites, launched from 1960 to 1962. Though only two of the five satellites made it into orbit, they returned a wealth of information on Soviet air defense radar capabilities as well as useful astronomical observations of the Sun.

Development

In 1957, the Soviet Union began deploying the S-75 Dvina surface-to-air missile, controlled by Fan Song fire control radars. This development made penetration of Soviet air space by American bombers more dangerous. The United States Air Force began a program of cataloging the rough location and individual operating frequencies of these radars, using electronic reconnaissance aircraft flying off the borders of the Soviet Union. This program provided information on radars on the periphery of the Soviet Union, but information on the sites in the interior of the country was lacking. Some experiments were carried out using radio telescopes looking for serendipitous Soviet radar reflections off the Moon, but this proved an inadequate solution to the problem. In March 1958, while the United States Naval Research Laboratory (NRL) was heavily involved in Project Vanguard, the United States Navy's effort to launch a satellite, NRL engineer Reid D. Mayo determined that a Vanguard derivative could be used to map Soviet missile sites. Mayo had previously developed an antenna system for submarines whereby they could evade anti-submarine aircraft by picking up their radar signals. Physically small and mechanically robust, it could be adapted to fit inside the small Vanguard frame. Mayo presented the idea to Howard Lorenzen, head of the NRL's countermeasures branch. Lorenzen promoted the idea within the Department of Defense (U.S. DoD), and six months later the concept was approved under the name "Tattletale". President Eisenhower approved full development of the program on 24 August 1959. When news of the project leaked in The New York Times, Eisenhower canceled the project. The project was restarted under the name "Walnut" (the satellite component given the name "DYNO") after heightened security had been implemented, including greater oversight and restriction of access to "need-to-know" personnel. American space launches were not classified at the time, and a cover mission that would share the satellite bus with DYNO was desired to conceal DYNO's electronic surveillance mission from its intended targets. The study of the Sun's electromagnetic spectrum provided an ideal cover opportunity. The Navy had wanted to determine the role of solar flares in radio communications disruptions and the level of hazard to satellites and astronauts posed by ultraviolet and X-ray radiation. Such a study had not previously been possible, as the Earth's atmosphere blocks much of the Sun's X-ray and ultraviolet output from ground observation. Moreover, solar output is unpredictable and fluctuates rapidly, making sub-orbital sounding rockets inadequate for the observation task. A satellite was required for long-term, continuous study of the complete solar spectrum. The NRL already had a purpose-built solar observatory in the form of Vanguard 3, which had been launched in 1959. Vanguard 3 had carried X-ray and ultraviolet detectors, though they had been completely saturated by the background radiation of the Van Allen radiation belt. Development of the DYNO satellite from the Vanguard design was managed by NRL engineer Martin Votaw, leading a team of Project Vanguard engineers and scientists who had not migrated to NASA. The dual-purpose satellite was renamed GRAB ("Galactic Radiation And Background"), sometimes called GREB ("Galactic Radiation Experiment Background"), and referred to in its scientific capacity as SOLRAD ("SOLar RADiation").

Operational history

The first GRAB satellite, SOLRAD 1, was launched 22 June 1960, on the same rocket as Transit 2A, an early naval navigation satellite. GRAB 1 had the distinction of being the first successful U.S. intelligence satellite, returning electronic intelligence (ELINT) data from 5 July 1960, until 22 September 1960, totaling 22 data collection passes of 40 minutes each over the Soviet Union, China and their allies. The SOLRAD experiment remained operational for ten months (though usable data was obtained only for five months) and it returned the first real-time X-ray and ultraviolet observations of the Sun. During the second launch attempt, the Thor booster shut down 12 seconds early, and the flight was subsequently terminated by range safety, raining fragments over Cuba. To ensure this did not happen again, subsequent launches from Cape Canaveral flew a dogleg trajectory to reach 70° inclination, avoiding the island nation. The other successful GRAB mission, GRAB 2, was launched 29 June 1961, atop the same Thor-Ablestar launch vehicle as Injun, a geophysical science satellite from the University of Iowa, and Transit 4A. GRAB 2 began transmission of intelligence to the ground on 15 July 1962, and functioned in orbit for fourteen months. The amount of data received was so large that automated analytic tools had to be developed, tools that found application in subsequent surveillance programs. GRAB 2's SOLRAD experiment (SOLRAD 3) also contributed substantially to solar X-ray astronomy. Three more GRAB satellites were produced, the first two failing to make orbit in 1962. The final scheduled GRAB flight was canceled, and the satellite intended for the mission was ultimately donated to the National Air and Space Museum in 2002.

Legacy The GRAB program formally ended with GRAB 2's last transmission in August 1962. After the establishment of the National Reconnaissance Office (NRO) in 1962, the GRAB program was succeeded by the POPPY program, which lasted from its funding authorization in July 1962 until its termination on 30 September 1977. The existence of the ELINT nature of GRAB was declassified by the NRL in 1998.

Table of launches

References

External links

GRAB at FAS GRAB at NRL Archived 23 July 2007 at the Wayback Machine SOLRAD/GRAB at NRL Archived 19 November 2011 at the Wayback Machine

Illustrations

Galactic Radiation and Background: This is a display model of a GRAB satellite at the National Cryptologic Museum.
This is a display model of a GRAB satellite at the National Cryptologic Museum.
Galactic Radiation and Background: SOLRAD 1 on top of Transit 2A with four of its creators.[1] From left: Martin J. Votaw, George G. Kronmiller, Alfred R. Conover, and Roy A. Harding.
SOLRAD 1 on top of Transit 2A with four of its creators.[1] From left: Martin J. Votaw, George G. Kronmiller, Alfred R. Conover, and Roy A. Harding.
Galactic Radiation and Background: GRAB 1 sitting atop Transit 2A during launch preparations.
GRAB 1 sitting atop Transit 2A during launch preparations.

Worked examples

Example 1 — a first encounter with Galactic Radiation and Background

Start with the simplest possible case. Write down what Galactic Radiation and Background claims or describes in one sentence, then invent the smallest concrete situation in which that sentence is true. In science, the smallest case is usually a single object, a single equation or a single measurement. Check that every symbol or term in your sentence has a meaning in that case.

Example 2 — changing one variable

Take the situation from Example 1 and change exactly one quantity: double it, halve it, or set it to zero. Predict what should happen to Galactic Radiation and Background before you calculate. Comparing your prediction with the result is the fastest way to find out whether you understand the idea or only the words.

Example 3 — an exam-style question

Typical questions about Galactic Radiation and Background ask you to (a) state it precisely, (b) apply it to given data, and (c) explain a limitation. Practise writing all three answers in under five minutes; the third part is what separates a full-mark answer from an average one.

Applications of Galactic Radiation and Background

In research
Galactic Radiation and Background appears in science research whenever the underlying quantities have to be modelled precisely. Papers usually cite it as a starting assumption and then explore where it breaks down.
In technology and industry
Engineering practice reuses Galactic Radiation and Background in design rules, simulations and safety margins. Knowing the idea lets you read a specification sheet and understand why the numbers look the way they do.
In the classroom
Galactic Radiation and Background is common in secondary-school and first-year university syllabi. It links to neighbouring topics 1962 in spaceflight, 1963 in spaceflight, Military equipment introduced in the 1960s, so understanding it makes those chapters shorter.
In everyday life
Look for Galactic Radiation and Background outside the textbook — in sport, cooking, traffic, electronics or the sky above you. An example you found yourself is remembered far longer than one you were given.
Ask Teacher Smith questions about this articleOpens your AI tutor with a question about “Galactic Radiation and Background” →

Affiliate

Preply — study more efficiently by working with a personal tutor. 50% off.

How to study Galactic Radiation and Background in 20 minutes

  1. Read the reference excerpt below once, without taking notes.
  2. Close the page and write down what Galactic Radiation and Background means in your own words.
  3. Compare your version with the excerpt and mark what you missed.
  4. Work through the three examples above with pen and paper.
  5. Explain Galactic Radiation and Background out loud to somebody else — or to Teacher Smith in the lgStudy chat.

Frequently asked questions

What is Galactic Radiation and Background in simple terms?

Galactic Radiation and Background (GRAB) was the first successful United States orbital surveillance program, comprising a series of five Naval Research Laboratory electronic surveillance and solar astronomy satellites, launched from 1960 to 1962. Though only two of the five satellites made it into…

Why does Galactic Radiation and Background matter?

Because it connects several science ideas at once: it gives you a definition you can apply, a quantity you can calculate, and a way to check whether a result is plausible.

How should I study Galactic Radiation and Background?

Read the excerpt, restate it from memory, then work through the examples and applications listed on this page. The five-step study plan above takes about twenty minutes.

What does this page cover?

It gives you a compact reference excerpt plus original lgStudy explanations, examples, applications and study material on Galactic Radiation and Background.

Tags

  • 1962 in spaceflight
  • 1963 in spaceflight
  • Military equipment introduced in the 1960s
  • National Reconnaissance Office
  • Reconnaissance satellites of the United States

Keep exploring