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Our Mr. Sun

Our Mr. Sun 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 Our Mr. Sun rather than just read about it. In short: Our Mr. Sun is a 1956 one-hour American television film in Technicolor written, produced, and directed by Frank Capra, with animation by UPA.

Our Mr. Sun — main illustration
Our Mr. Sun — illustration

Key takeaways

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

Reference excerpt

Our Mr. Sun is a 1956 one-hour American television film in Technicolor written, produced, and directed by Frank Capra, with animation by UPA. It is a documentary that explains how the Sun works and how it also plays a huge part in human life. It was first broadcast on television by CBS in 1956. The film starred Frank Baxter as "Dr. Research", and Eddie Albert as "the fiction writer", the other recurring character in The Bell Laboratory Science Series. Marvin Miller voiced the animated Sun. Sterling Holloway, who was uncredited, voiced an animated version of chlorophyll. The film is notable as the last project of actor Lionel Barrymore, who provided the voice of Father Time. The film was first broadcast on television two years after Barrymore's death in 1954. Our Mr. Sun and a companion film, Hemo the Magnificent (about blood circulation), were popular favorites for showing in primary and secondary school science classrooms from the late 1950s until the early 1980s. The film is currently available on DVD with another Frank C. Baxter film, The Strange Case of the Cosmic Rays (1957).

Synopsis The film opens with Dr. Research (Dr. Frank C. Baxter) and the Fiction Writer (Eddie Albert) meeting Father Time (Lionel Barrymore) and Mr. Sun (Marvin Miller) who explain that time started a few billion years ago and that the Sun is a star. Mr. Sun explains that he was worshipped as various gods (Shamash, Mithra, Ra and Apollo) until Anaxagoras proclaimed the Sun was a very hot stone and not a god. Logic and reasoning were the beginning of the end of worshiping the Sun as algebra and the astrolabe were used to study the heavens. Dr. Research explains that the Sun is 93 million miles away and its light takes 8 minutes to reach the Earth. Light from the next closest star, Alpha Centauri, takes more than 4 years to get to Earth at a speed greater than 186,000 miles per second. The Sun weighs the same as about 330,000 Earths and is 95% hydrogen and helium gas and is not solid. The Sun is compressed by gravity so tightly that the gas at the center is more than 100 times heavier than water with a pressure of one billion tons per square inch while the surface is about one pound per square inch. The center of the Sun is 30 million degrees Fahrenheit while the surface is only 10,000 degrees, but the corona is 1 million degrees Fahrenheit though nobody knows why, so scientists study the Sun's corona during each solar eclipse. Dr. George Ellery Hale and Dr. Henri Deslandres both developed the spectroheliograph—independently—to study the Sun in different wavelengths of light related to specific atoms. Dr. Robert R. McMath of the McMath–Hulbert Observatory used a spectroheliograph to make time-lapse films of the prominences on the Sun. Using pictures from the Mount Wilson Observatory, and others, scientists have learned about sunspots first described by Galileo. Sunspots often appear in pairs and are about 7,000 degrees rather than the normal 10,000 degrees. The spots increase and decrease in a cycle of about 11.2 years. Studying sunspots has shown the equator rotates faster than the poles at around 25 and 1/3 days per rotation. Halfway between the equator and the poles takes about 27 and 1/2 days per rotation though nobody understands why.

… excerpt ends here. Continue reading the full article.

Worked examples

Example 1 — a first encounter with Our Mr. Sun

Start with the simplest possible case. Write down what Our Mr. Sun 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 Our Mr. Sun 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 Our Mr. Sun 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 Our Mr. Sun

In research
Our Mr. Sun 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 Our Mr. Sun 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
Our Mr. Sun is common in secondary-school and first-year university syllabi. It links to neighbouring topics 1950s educational films, 1956 English-language films, 1956 documentary films, so understanding it makes those chapters shorter.
In everyday life
Look for Our Mr. Sun 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.
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How to study Our Mr. Sun in 20 minutes

  1. Read the reference excerpt below once, without taking notes.
  2. Close the page and write down what Our Mr. Sun 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 Our Mr. Sun out loud to somebody else — or to Teacher Smith in the lgStudy chat.

Frequently asked questions

What is Our Mr. Sun in simple terms?

Our Mr. Sun is a 1956 one-hour American television film in Technicolor written, produced, and directed by Frank Capra, with animation by UPA.

Why does Our Mr. Sun 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 Our Mr. Sun?

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 Our Mr. Sun.

Tags

  • 1950s educational films
  • 1956 English-language films
  • 1956 documentary films
  • 1956 films
  • 1956 television films
  • American documentary television films
  • American educational films
  • Documentary films about science
  • English-language documentary films
  • English-language television films
  • Films directed by Frank Capra
  • Sponsored films

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