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Vesto Slipher

Vesto Slipher 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 Vesto Slipher rather than just read about it. In short: Vesto Melvin Slipher (; November 11, 1875 – November 8, 1969) was an American astronomer who performed the first measurements of radial velocities for galaxies. He was the first to discover that distant galaxies are redshifted, thus providing the first empirical basis for the expansion of the universe.

Vesto Slipher — main illustration
Vesto Slipher — illustration

Key takeaways

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

Reference excerpt

Vesto Melvin Slipher (; November 11, 1875 – November 8, 1969) was an American astronomer who performed the first measurements of radial velocities for galaxies. He was the first to discover that distant galaxies are redshifted, thus providing the first empirical basis for the expansion of the universe. He was also the first to relate these redshifts to velocity.

Early life and education Vesto Melvin Slipher was born in Mulberry, Indiana, to Daniel Clark and Hannah App Slipher. He spent his early years working on his family farm in Mulberry. Vesto had a younger brother, Earl C. Slipher, who was also an astronomer at Lowell Observatory. Slipher went to high school in Frankfort, Indiana. He then attended Indiana University Bloomington and earned his Bachelor's Degree in Mechanics and Astronomy in June 1901. Two years later, Slipher earned his Master's Degree in the same program. At the age of 33, Vesto graduated with his Ph.D. in Mechanics and Astronomy from Indiana University.

Career While at school at Indiana University, Slipher formed a personal bond with one of his professors, William Cogshall. Cogshall was one of the main reasons Slipher became interested in astronomy in the first place. Cogshall convinced Percival Lowell, director of the Lowell Observatory in Flagstaff, Arizona, to take Vesto in as a temporary assistant. Slipher worked as an assistant from 1901 to 1915 when Lowell finally named him the assistant director of the observatory. One year later Percival Lowell died and Vesto became the acting director for the next ten years. In 1926, 25 years after arriving in Flagstaff, Slipher was named director of the Lowell Observatory. He remained in charge for 28 more years when he retired from professional life. Slipher spent his years there studying many things, but most notably, spectroscopy and redshifts of spiral nebulae. The first major task Slipher was given was to measure the Solar System's planets' rotation interval. He was one of the first astronomers to show that Uranus has a much faster rotation than Earth, similar to the other giant planets in the Solar System. What Vesto is most known for though is his work with spiral nebulae, or, spiral galaxies, like the Milky Way and Andromeda. His initial goal was to measure how fast the nebulae were moving. His discoveries were confirmed ten years later when Edwin Hubble used the Mount Wilson Observatory reflector to view the galaxies much more clearly.

Discoveries

Slipher introduced as early as 1909 that the infrared spectrum could be recorded using photographic emulsions, and used those to record the absorption lines of sunlight and major planets. He found that the planets showed different absorption lines that were not present in sunlight, and identified those bands with ammonia and methane. In the early twentieth century, Vesto Slipher elongated the spectrum to include the red and infrared wavelengths and showed that the major planets display strong absorption lines at many different wavelengths..> Slipher used spectroscopy to investigate the rotation periods of planets and the composition of planetary atmospheres. In 1912, he was the first to observe the shift of spectral lines of galaxies, making him the discoverer of galactic redshifts. Using the Doppler effect and noting subtle changes, he measured the speeds in which spiral nebulae traveled during his research from 1912 and onward. These subtle changes in the speeds of the nebulae led Slipher to conclude that the nebulae were not within the Milky Way galaxy. In 1914, Slipher also made the first discovery of the rotation of spiral galaxies. He discovered the sodium layer in 1929. He was responsible for hiring Clyde Tombaugh and supervised the work that led to the discovery of Pluto in 1930. By 1917, Slipher had measured the radial velocities of 25 "spiral nebulae," and found that all but three of those galaxies were moving away from us, at substantial speeds. Slipher himself speculated that this might be due to the motion of our own galaxy – as in his sample, those galaxies moving towards us and those moving away from us were roughly in opposite directions. In hindsight, this was the first data supporting models of an expanding universe. Later, Slipher's and additional spectroscopic measurements of radial velocities were combined by Edwin Hubble with Hubble's own determinations of galaxy distances, leading Hubble to discover the (at that time, rough) proportionality between galaxies' distances and redshifts, which is today termed the Hubble–Lemaître law (formerly named Hubble's law; the IAU Decision of October 2018 recommends the use of a new name), was formulated by Hubble and Humason in 1929 and became the basis for the modern model of the expanding universe.

Personal life Slipher married Emma R. Munger in 1904 in Frankfort, Indiana. Vesto and Emma had two children – David Clark and Marcia Frances. In 1901 Slipher moved to Flagstaff, Arizona, and began work at Lowell Observatory. He continued at Lowell as an assistant and as the director until his retirement in 1954. Slipher died in Flagstaff in 1969 at age 93. He is buried at Citizens Cemetery in Flagstaff.

Awards Member of the American Academy of Arts and Sciences (elected 1909) Lalande Prize (1919) Gold Medal of the Paris Academy of Sciences (1919) Member of the United States National Academy of Sciences (1921) Member of the American Philosophical Society (1921) Henry Draper Medal of the National Academy of Sciences (1932) Gold Medal of the Royal Astronomical Society (1932) Bruce Medal (1935) The crater Slipher on the Moon is named after Earl and Vesto Slipher, as is the crater Slipher on Mars and the asteroid 1766 Slipher, discovered September 7, 1962, by the Indiana Asteroid Program.

References

Sources Gingerich, Owen; Lang, Kenneth R., eds. (1979). A Source Book in Astronomy and Astrophysics, 1900–1975. Cambridge, Massachusetts and London: Harvard University Press. ISBN 0-674-82200-5. OCLC 3933662. Hoyt, William Graves (1980). "Vesto Melvin Slipher". In Crawford Jr., Bryce; McEuen, Caroline K. (eds.). Biographical Memoirs of the National Academy of Sciences. Vol. 52. Washington D.C.: National Academies Press. pp. 411–449. ISBN 0-309-03099-4 – via Internet Archive.

External links Library of Lowell Observatory: Biography of V. M. Slipher The Royal Observatory, Edinburgh: History, Papers & External Links on V. M. Slipher Vesto Melvin Slipher at Find a Grave V. Slipher @ Astrophysics Data System

Worked examples

Example 1 — a first encounter with Vesto Slipher

Start with the simplest possible case. Write down what Vesto Slipher 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 Vesto Slipher 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 Vesto Slipher 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 Vesto Slipher

In research
Vesto Slipher 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 Vesto Slipher 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
Vesto Slipher is common in secondary-school and first-year university syllabi. It links to neighbouring topics 1875 births, 1969 deaths, 20th-century American astronomers, so understanding it makes those chapters shorter.
In everyday life
Look for Vesto Slipher 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 Vesto Slipher in 20 minutes

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

Frequently asked questions

What is Vesto Slipher in simple terms?

Vesto Melvin Slipher (; November 11, 1875 – November 8, 1969) was an American astronomer who performed the first measurements of radial velocities for galaxies. He was the first to discover that distant galaxies are redshifted, thus providing the first empirical basis for the expansion of the unive…

Why does Vesto Slipher 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 Vesto Slipher?

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 Vesto Slipher.

Tags

  • 1875 births
  • 1969 deaths
  • 20th-century American astronomers
  • Fellows of the American Academy of Arts and Sciences
  • Indiana University Bloomington alumni
  • Members of the American Philosophical Society
  • Members of the United States National Academy of Sciences
  • People from Clinton County, Indiana
  • People from Flagstaff, Arizona
  • Recipients of the Gold Medal of the Royal Astronomical Society
  • Recipients of the Lalande Prize

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