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Fred Lawrence Whipple

 
Scientist: Fred Lawrence Whipple

American astronomer (1906–2004)

Born in Red Oak, Iowa, Whipple graduated from the University of California in Los Angeles in 1927 and obtained his PhD from Berkeley in 1931. He then moved to Harvard where he became professor of astronomy in 1945, Philips Professor of Astronomy in 1950, and director of the Smithsonian Astrophysical Observatory from 1955 until his retirement in 1973.

He described his research as centering on “physical processes in the evolution of the solar system” and produced in this field a much admired work, Earth, Moon and Planets (1941 and many subsequent editions).

Whipple is also well known for his work on comets. In 1950 he proposed an icy-nucleus model in which he described the nucleus of a comet as a ‘dirty snowball’, made from a mixture of water ice and dust, plus carbon dioxide, carbon monoxide, methane, and ammonia ices, and only becoming active when passing close to the Sun. The main advantage of this model is that it can account for such distinctive features of comets as their orbital motion. It had been long known that some comets, such as Encke's, persist in returning earlier than Newtonian theory would predict while others, such as Halley's, arrive over four days later than expected. Whipple proposed that solar radiation would cause the ices on the outside of the cometary nucleus to evaporate, leaving a thin insulating layer of dust particles, and that this would set up a delayed jet reaction. The radiation has the effect of pushing further out those comets that are rotating in the same direction as their orbit. This will increase their orbit and delay their return. The radiation will produce a drag force on those comets rotating counter to their orbit, causing them to drift in toward the Sun, reducing their period and thus hastening their return.

As there should be no preferred direction of rotation, Whipple predicted that about half the comets should appear to be retarded and half accelerated in their orbit, an effect since confirmed.

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Biography: Fred Lawrence Whipple
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During his lifetime, American astronomer Fred Whipple (1906 - 2004) was recognized as the world's leading expert on solar system astronomy. Before Whipple came along, scientists believed comets were nothing more than loose clouds of dusty vapor held together by gravity. In 1950, however, Whipple proposed that comets were really enormous rock - embedded ice balls surrounded by gas and dust. His so - called "dirty snowball" theory remained controversial until 1986, when a spacecraft photographed the icy contents of Halley's comet, proving Whipple's 36 - year - old theory to be accurate. Besides comets, Whipple dedicated his life to studying other components of the solar system. His work helped scientists around the globe better understand the universe and also helped pave the way for spaceflight.

Discovered Astronomy in College

Whipple was born November 5, 1906, in Red Oak, Iowa, to farmers Harry Lawrence and Celestia (MacFarland) Whipple. When he was in his teens, the Whipples left the family farm and relocated to Long Beach, California. Once there, Whipple worked as a clerk in his father's grocery store. He graduated from Long Beach High School in 1923. From 1923 - 24, Whipple studied at Occidental College in Los Angeles, California, and dreamed of a career in tennis. He later transferred to the University of California at Los Angeles (UCLA).

In an August 2000 issue of Science, Whipple wrote about his childhood. "As an Iowa farm boy, I contracted a case of polio and it prevented me from becoming a professional tennis player. When I entered the University of California at Los Angeles, it was still my main ambition to excel at tennis. A mathematics major enabled me to bring home good grades without having to spend much time on studies. But I never made the tennis team."

During his junior year at UCLA, Whipple took a course from famed astronomer Frederick Leonard, founder of the Meteoritical Society. Studying the science of the universe and its matter intrigued Whipple. He began to focus more on astronomy and less on mathematics, though he completed his studies in mathematics, earnings his degree in 1927. By then, it had become clear to Whipple that he had to give up his dream of playing professional tennis. Instead, he turned his full attention to astronomy and with Leonard's help, secured a teaching fellowship in astronomy at the University of California at Berkeley.

While studying at Berkeley, Whipple learned how to compute the orbits of celestial bodies, such as meteors, comets and planets. He was part of a team that calculated the orbit of the newly discovered planet Pluto. After graduating with his doctorate in astronomy in 1931, Whipple became head of the observing program at the Harvard College Observatory. Once there, he stayed for more than 70 years. When Whipple first went to Harvard, he was interested in studying galaxies, but his boss made it clear that he would be the one studying galaxies. Whipple decided to focus his attention on comets; it became the pursuit of a lifetime. Whipple cautiously examined the "sky - patrol" photographs taken regularly at the observatory and over the course of a decade, discovered six new comets and computed their orbits. He also began to study the behavior of comets, photographing them as they moved in their egg - shaped orbits around the sun.

Helped WWII Bombers Trick Enemy Radar

After the United States became involved in World War II, Whipple left the observatory to work in the office of scientific research and development at the Harvard Radio Research Laboratory. He stayed there from 1942 - 45. During this time, Whipple worked on radar countermeasures. He co - invented a razor - sharp device that cut aluminum foil into tiny slices called chaff, which were dropped by bombers as they approached enemy radar, thus confusing the readings. Dropping the aluminum slices made it appear like there were more aircraft in the sky than in reality. In 1948, Whipple earned a Presidential Certificate of Merit for this invention.

After the war, Whipple returned to the Harvard observatory and his study of comets. He believed spaceflight was just around the corner and in 1946, Whipple invented a "meteor bumper" to protect spacecraft and satellites from collisions with space debris. The device, known as the "Whipple shield," is made up of thin layers of metal that surround the body of a spacecraft a few inches out from its surface. The bumper absorbs the impact when the craft strikes another object. As the 21st century began, the device - with some updates - was still being used on virtually every interplanetary spacecraft put into orbit. Whipple thought of himself as part inventor, part astronomer. Reading his 2004 obituary in the Boston Globe, this is clear: "I'm an engineer at heart," he once remarked, according to the paper. "I've been able to judge what instruments will work and what can be built. That's been the secret to my success."

Developed "Dirty Snowball" Theory of Comets

As Whipple continued his study of comets, it became clear to him that comets had an icy core. At the time, most scientists believed comets were merely dusty orbiting clouds of vapor, sand and rock. Comets were thought of as "floating sandbanks" held loosely together by gravity with no solid core. A minority of scientists believed comets were rocks spewed out by volcanoes on Jupiter and Saturn. The comet's spectacular tail had also troubled scientists. It seemed impossible to think that a comet had enough material to keep emitting its tale without getting smaller and smaller and eventually disappearing. Whipple theorized that comets were really balls of gas, rock and dust with an icy nucleus. He published his so - called "dirty snowball" theory in the March 1950 issue of the Astrophysical Journal. Controversy ensued.

During his studies, Whipple discovered that comets did not act like other bodies in the solar system. They did not adhere to the simple Newtonian mechanics of other bodies - they weren't predictable. Some comets reached the Earth earlier than expected; others were late. Because of this, Whipple theorized that some unknown force - besides gravity - was affecting the comets. Whipple believed that comets were really large masses of dust and ice that vaporized as the comet approached the sun and refroze as it receded from the sun. He theorized that when a comet approached the sun and began to evaporate, it released its frozen water. This trail of vapor not only produced the fabulous tail but also caused propulsion jets that propelled the comet forward, at times altering its orbit. Whipple's theory was much - debated until 1986, when the European Space Agency's Giotto spacecraft got near Halley's comet and snapped pictures of an icy core, proving his theory.

Whipple's idea was "one of the most important contributions to solar system studies" in the twentieth century, Smithsonian Astrophysical Observatory astronomer Brian Marsden told Boston Globe staff writer David Chandler.

What amazed Whipple's colleagues most about his discovery was that Whipple made the conceptual leap based mostly on intuition, sparked by a little data. Speaking to the Los Angeles Times, Harvard - Smithsonian Center astrophysicist Mike Lecar summed up Whipple's significance this way: "Unlike other great physicists, he had uncommon common sense. He just looked at things with a fresh eye."

By 1950, Whipple was a full Harvard professor of astronomy. In 1955, he also became director of the Smithsonian Astrophysical Observatory after it moved from Washington, D.C., to Cambridge, Massachusetts. He held that position until 1973. During his years at Harvard, Whipple wrote many papers and books and inspired many future scientists, including astronomer Carl Sagan, whose 1980 PBS series "Cosmos" helped popularize astronomy. Whipple's 1941 book, Earth, Moon and Planets, also popularized the study of the skies by explaining solar system astronomy to the masses.

Whipple was also one of the first scientists to envision the coming age of satellites. In the late 1950s, he set up a satellite tracking program called "Moonwatch." Participating in the program were several observing stations around the world, all equipped with special sky - watch cameras, and a network of amateur astronomers who volunteered to watch the skies. When the former Soviet Union launched Sputnik, the first artificial satellite, in 1957, Whipple's "Moonwatch" team was able to track its progress around the globe. Virtually all information about the satellite that went to the media and public came from Whipple's "Moonwatch" program. President John F. Kennedy presented Whipple with the Distinguished Federal Civilian Service Award in 1963 for this work. At the time of the launch, tensions between the Soviet Union and the United States ran high. U.S. citizens were concerned about having the Russian satellite fly over their country, but Whipple's data eased fears. Whipple was proudest of the award he received for this work. "I think that was my most exciting moment, when I was able to invite my parents and my family to the Rose Garden for the ceremony," he once said, according to the Los Angeles Times.

During the late 1960s, Whipple joined fellow astronomer Aden Meinel in creating the first multiple - mirrored telescope. It started when Meinel told Whipple about six large telescope mirrors the Air Force was getting rid of. Working together, the two invented a multiple - mirror telescope, which collected light from the six mirrors, then focused it onto a single camera. Synthesizing the light from the six mirrors into one image made the telescope perform like a much larger telescope than it was. The multiple - mirror telescope, located on Arizona's Mt. Hopkins, was dedicated in 1979. It held the honor of being the world's third - largest telescope for two decades. In 1982, the Mt. Hopkins Observatory was renamed the Fred Lawrence Whipple Observatory.

Continued Work into his 90s

Over the course of his career, Whipple made many contributions to the field of astronomy. Besides determining what comets are made of, he also figured out that meteors are made of particles that come from within our solar system, rather than from particles arriving from outside the solar system, as some believed. Whipple also used satellite data to learn about the Earth's upper atmosphere and its daily changes. In addition, he helped advance the types of technology used in studying space. In 1968, the world's first space telescope, called the Orbiting Astronomical Observatory, was launched, thanks to Whipple. Though this telescope had a mechanical malfunction that led to its failure, it helped pave the way for the Hubble Space Telescope. "Fred had the vision very early about a telescope in space," Eugene Shoemaker told the Boston Globe's Chandler. "He was talking about this before there was a NASA." For his many contributions to our understanding of the solar system, minor planet No. 1940 was named after Whipple in 1975.

Whipple retired in 1977, though as a professor emeritus, he continued his daily treks to his Cambridge, Massachusetts, office. Until he turned 90, he biked the three miles to his office nearly every day. He continued his work at the observatory almost until the end of his life. Whipple was well - known in the Cambridge area - easily identified driving his car, whose license plate read COMET.

Whipple died August 30, 2004, in Cambridge. He was 97. Whipple was survived by his first wife, Dorothy Woods, and their son, Earle. Whipple and Woods married in 1928 and divorced in 1935. He was also survived by his second wife, Babette Samelson, whom he married in 1946. They had two children, Sandra and Laura.

Periodicals

Boston Globe, October 28, 1996; August 31, 2004.

Guardian (London), September 2, 2004.

Independent (London), November 13, 2004.

Los Angeles Times, September 1, 2004.

Science, August 4, 2000.

Times (London), September 4, 2004.

 
Columbia Encyclopedia: Fred Lawrence Whipple
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Whipple, Fred Lawrence, 1906-2004, American astronomer, b. Red Oak, Iowa. After graduating from the Univ. of California, Berkeley (Ph.D. 1931), he accepted a position at Harvard, where he remained for the rest of his career. During World War II he helped develop the aluminum chaff that was used to confuse enemy radar, but he is best known for proposing in a 1950 paper that comets were frozen gases with other substances mixed in, not unlike a "dirty snowball." Whipple, who headed the Smithsonian Astrophysical Observatory from 1955 to 1973, also anticipated artificial satellites, establishing an early tracking station before the first Sputnik launch (1957).
Wikipedia: Fred Lawrence Whipple
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Fred Lawrence Whipple

Fred Lawrence Whipple aged 95
Born November 5, 1906
Red Oak, Iowa
Died August 30, 2004
Nationality American
Fields astronomy
Institutions Harvard College Observatory
Known for comets composition

Fred Lawrence Whipple (November 5, 1906–August 30, 2004) was an American astronomer, who worked at the Harvard College Observatory for over 70 years. Amongst his achievements, he discovered some asteroids and comets, came up with the "dirty snowball" cometary hypothesis, and designed the Whipple shield.

Contents

Life

Whipple was born on November 5, 1906, in Red Oak, Iowa, as the son of a farmer. An early bout with polio ended his ambition of being a professional tennis player. Whipple studied at Occidental College in Southern California, then majored in mathematics at the University of California at Los Angeles, graduating in 1927.

After taking a class in astronomy, he enlisted at the University of California, Berkeley where he obtained his PhD in Astronomy in 1931. While in graduate school, he helped map the orbit of the newly discovered planet Pluto. He joined Harvard College Observatory in 1931 and studied the trajectories of meteors, confirming that they originated within the solar system rather than from interstellar space. In 1933, he discovered the periodic comet 36P/Whipple and the asteroid 1252 Celestia. He also discovered or co-discovered five other non-periodic comets, the first of which was C/1932 P1 Peltier-Whipple, independently discovered by the famed amateur astronomer Leslie Peltier.

During World War II, he invented a device for cutting tinfoil into chaff to confuse enemy radar tracking Allied aircraft. He was awarded a Certificate of Merit for this in 1948. He also invented a "meteor bumper" or "Whipple shield", which protects spacecraft from impact by small particles by vaporizing them.

From 1950 until 1977 he was a professor of Astronomy at Harvard University, including being the Phillips Professor of Astronomy between 1968 and 1977. During these years (in the early 1950s), he wrote a series of influential papers entitled A Comet Model, published in Astrophysical Journal.[1][2][3]. In these papers, he proposed the "icy conglomerate" hypothesis of comet composition (later called the "dirty snowball" hypothesis). The basic features of this hypothesis were later confirmed, however the exact amount (and thus the importance) of ices in a comet is an active field of research, with most of the recently obtained data[4] pointing to a low contribution of ices to a comet's mass (dubbed the "icy dirtball" hypothesis). He also anticipated the era of artificial satellites and organized the members of Operation Moonwatch to track them. These groups were the only ones prepared and ready to make observations when the Soviet Union unexpectedly launched Sputnik I in 1957. In 1955 he became director of the Smithsonian Astrophysical Observatory, remaining in this post until 1973.

Whipple died in 2004, aged 97, after prolonged illness.

Honors

Awards

Named after him

References

  1. ^ Whipple, Fred L. (1950). "A Comet Model. I. The acceleration of Comet Encke". Astrophysical Journal 111: 375–394. doi:10.1086/145272. http://adsabs.harvard.edu//full/seri/ApJ../0111//0000375.000.html. 
  2. ^ Whipple, Fred L. (1951). "A Comet Model. II. Physical Relations for Comets and Meteors". Astrophysical Journal 113: 464. doi:10.1086/145416. http://adsabs.harvard.edu//full/seri/ApJ../0113//0000464.000.html. 
  3. ^ Whipple, Fred L. (1955). "A Comet Model. III. The Zodiacal Light". Astrophysical Journal 121: 750. doi:10.1086/146040. http://adsabs.harvard.edu//full/seri/ApJ../0121//0000750.000.html. 
  4. ^ Keller, Horst Uwe et al. (2005). "Deep Impact Observations by OSIRIS Onboard the Rosetta Spacecraft". Science 310: 281. doi:10.1126/science.1119020. PMID 16150976. 

Further reading

External links


 
 
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Fred Lawrence Whipple Observatory (structure, Arizona – in astronomy)
Mount Hopkins (Arizona)
telescope (system, mechanical device – in optics)

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Scientist. A Dictionary of Scientists. Copyright © Market House Books Ltd 1993, 1999, 2003. All rights reserved.  Read more
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