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Henrietta Hill Swope

Henrietta Hill Swope is a astronomy 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 Henrietta Hill Swope rather than just read about it. In short: Henrietta Hill Swope (October 26, 1902 – November 24, 1980) was an American astronomer who studied variable stars. In particular, she measured the period-luminosity relation for Cepheid stars, which are bright variable stars whose periods of variability relate directly to their intrinsic luminosities.

Henrietta Hill Swope — main illustration
Henrietta Hill Swope — illustration

Key takeaways

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

Reference excerpt

Henrietta Hill Swope (October 26, 1902 – November 24, 1980) was an American astronomer who studied variable stars. In particular, she measured the period-luminosity relation for Cepheid stars, which are bright variable stars whose periods of variability relate directly to their intrinsic luminosities. Their measured periods can therefore be related to their distances and used to measure the size of the Milky Way and distances to other galaxies.

Personal life She was the daughter of Mary Hill and Gerard Swope, and niece of Herbert Bayard Swope. Both of her parents taught at Hull-House in Chicago in the late 1890s, where they met. Her father had attended MIT and was an engineer. He worked for General Electric, eventually rising to be president of the company in 1922 and enabling his daughter to be independently wealthy throughout her life. She learned of talks at Maria Mitchell Observatory while vacationing with her family on Nantucket, and took an evening class there alongside her brother. She also heard Harvard astronomer Harlow Shapley speak; eventually she would go to work with him on variable stars.

Education Swope attended Barnard College, and graduated in 1925, with an AB degree in mathematics. She only took an astronomy class, from Harold Jacoby, in her final year. After college, she went back to Chicago and attended the School of Social Service Administration, at the University of Chicago, but only for one year. While working with Harlow Shapley, she obtained her Masters in Astronomy in 1928 from Radcliffe College.

Professional history She learned that Dr. Shapley at Harvard was offering fellowships for women to work on finding variable stars. Swope went to work for Shapley in 1926 and began working alongside other "girls" to identify variable stars in the Milky Way. She became friends with Cecilia Payne-Gaposchkin and Adelaide Ames. She supported herself on a salary from Harvard and a stipend from her family. She became an expert on estimating magnitudes of stars from images on photographic plates. Swope left Harvard to work for MIT's staff Radiation Laboratory in 1942. In her Oral History, she says, "...they said, 'How much were you getting [at Harvard]?' And I said, I think, $2000. That’s what they say they would pay me, what I was getting, but that was too little for them. They couldn't. So I rose fairly quickly." From 1942-1947, she worked on the LORAN navigation tables. From 1947 until 1952, Swope taught astronomy at Barnard College and Connecticut College for Women and did research using old plates from Harvard. In 1952, Walter Baade of the Carnegie Institution of Washington's Observatories asked her, via Martin Schwarzschild as an intermediary, to come work with him on variable stars detected in other galaxies by the new 200-inch Hale Telescope at Palomar Observatory. Although she was hired as Baade's research assistant, in the "nebular-studies" group, she worked independently even to the point of writing scientific publications with his name on them after his death. She stayed at the Carnegie Institution for the rest of her career; she officially retired in 1968. In 1964, a paper by Baade & Swope reported the results of light curves for 275 Cepheids derived by Swope from photographic plates of the Andromeda Galaxy taken at the relatively new Hale 200-inch Telescope at Palomar Mountain. They reported a new distance to M31, given as a distance modulus of 24.25. They followed up this work in 1963 with new results of 20 Cepheids in a region of Andromeda less affected by extinction and estimated a new distance modulus of 24.20 mag.

Legacy In 1967, Swope made a donation of securities valued at $650,000 to the Carnegie Institution of Washington to develop "optical astronomical observatory facilities in the Southern Hemisphere." This gift was used for development of the site, including roads, water, and power systems, and for building a 40-inch telescope at Carnegie's Las Campanas Observatory in Chile. This telescope was named the Swope Telescope in her honor; it started operation in 1971 and is still used today. Swope also left most of her estate to Carnegie to support further Las Campanas and astronomical research at the institution more generally. Henrietta Hill Swope died at the age of 78 in Pasadena in California.

Awards and honors Annie J. Cannon Award in 1968 Asteroid 2168 Swope is named in her honor. Barnard Distinguished Alumnae Award, 1975 The Swope Telescope at the Las Campanas Observatory in Chile is named in her honor. Honorary PhD, 1975, University of Basel, Switzerland Barnard College Medal of Distinction, 1980

References

External links Henrietta Hill Swope Papers.Schlesinger Library Archived 2012-05-09 at the Wayback Machine, Radcliffe Institute, Harvard University. Oral history interview transcript with Henrietta Hill Swope on 3 August 1977, American Institute of Physics, Niels Bohr Library & Archives

Illustrations

Henrietta Hill Swope illustration

Worked examples

Example 1 — a first encounter with Henrietta Hill Swope

Start with the simplest possible case. Write down what Henrietta Hill Swope claims or describes in one sentence, then invent the smallest concrete situation in which that sentence is true. In astronomy, 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 Henrietta Hill Swope 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 Henrietta Hill Swope 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 Henrietta Hill Swope

In research
Henrietta Hill Swope appears in astronomy 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 Henrietta Hill Swope 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
Henrietta Hill Swope is common in secondary-school and first-year university syllabi. It links to neighbouring topics 1902 births, 1980 deaths, 20th-century American astronomers, so understanding it makes those chapters shorter.
In everyday life
Look for Henrietta Hill Swope 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 Henrietta Hill Swope in 20 minutes

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

Frequently asked questions

What is Henrietta Hill Swope in simple terms?

Henrietta Hill Swope (October 26, 1902 – November 24, 1980) was an American astronomer who studied variable stars. In particular, she measured the period-luminosity relation for Cepheid stars, which are bright variable stars whose periods of variability relate directly to their intrinsic luminositi…

Why does Henrietta Hill Swope matter?

Because it connects several astronomy 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 Henrietta Hill Swope?

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 Henrietta Hill Swope.

Tags

  • 1902 births
  • 1980 deaths
  • 20th-century American astronomers
  • 20th-century American women scientists
  • American women astronomers
  • Barnard College alumni
  • Crown Family School of Social Work, Policy, and Practice alumni
  • MIT Radiation Laboratory people
  • Radcliffe College alumni
  • Recipients of the Annie J. Cannon Award in Astronomy
  • Scientists from St. Louis

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