Gerard Peter Kuiper

  • Born: December 7, 1905
  • Birthplace: Harenkarspel, the Netherlands
  • Died: December 23, 1973
  • Place of death: Mexico City, Mexico

Dutch American astronomer

Twentieth-century Dutch American astronomer Gerard Peter Kuiper was a leading planetary scientist. He taught and conducted research at a number of major American astronomical installations, inspired the construction of several observatories, contributed significantly to early NASA moon-exploration projects, and made many discoveries within the solar system.

Born: December 7, 1905; Tuitjenhorn, Netherlands

Died: December 24, 1973; Mexico City, Mexico

Also known as: Gerrit Pieter Kuiper

Primary field: Astronomy

Specialties: Observational astronomy; astrophysics; theoretical astronomy

Early Life

Gerard Peter Kuiper was born as Gerrit Pieter Kuiper in a village in North Holland. He was the eldest of four children born to tailor Gerrit Kuiper and his wife, Antje de Vries. Kuiper became interested in astronomy as a child, thanks to his grandfather, who gave him a telescope as a present. From boyhood, he was gifted with exceptional eyesight, capable of spotting with his naked eye faint stars that most people could not see without magnification.

An eager student, Kuiper attended grade school in his hometown. For secondary school, he went to a teaching preparatory facility in Haarlem, near Amsterdam, after which he was certified to teach mathematics at the secondary school level. Following graduation, he passed the entrance examination for Leiden University and enrolled in 1924, majoring in theoretical physics with a concentration in astronomy. There, Kuiper and fellow students—and future astronomers—Bart Bok and Piet Oosterhoff together took classes from such outstanding teachers as physicist Paul Ehrenfest, chemist-astronomer Ejnar Hertzsprung, astronomers Jan Oort and Antonie Pannekoek, and mathematician-physicist-astronomer Willem de Sitter. Kuiper was particularly interested in binary stars; he published his first scholarly paper on the subject in 1926.

Kuiper earned a bachelor of science degree in 1927 and embarked on postgraduate studies at the university. In 1929, he traveled to the Dutch East Indies (later Indonesia) to work on an eight-month solar eclipse project at the Bosscha Observatory in West Java. By 1933, when Kuiper received his PhD, he had more than a dozen articles in scientific journals to his credit. After finishing his doctoral studies, he traveled to the United States on fellowships to work on a detailed survey of binary stars and white dwarf stars under astronomer Robert Grant Aitken at Lick Observatory at the University of California, Santa Cruz.

Life’s Work

Kuiper left Lick in 1935 to work at Harvard University’s Oak Ridge Observatory, which had opened in 1933 and boasted the largest telescope on the East Coast. He intended to conduct studies for a year before returning to Java; however, while at Harvard, Kuiper met Sarah Parker Fuller, daughter of the family that had donated land for the observatory. The couple married in 1936 and would have two children, Paul (born 1941) and Sylvia (born 1947).

After their wedding, Kuiper and his wife relocated to the University of Chicago, where he became a professor and staff astronomer at Yerkes Observatory. In 1937, he became an American citizen. He was a member of the planning committee for the new McDonald Observatory, a joint Yerkes–University of Texas facility that featured an eighty-two-inch reflecting telescope. After the observatory opened in 1939, Kuiper and his wife moved to Texas, where he continued his study of binary stars.

During the last two years of World War II, Kuiper worked for the US government at the secret Harvard Radio Research Laboratory, which developed devices to deceive Axis powers’ radar and disrupt communications. In the course of his wartime duties, Kuiper made several trips to Europe. He was involved with the Allies’ Alsos Mission, a top-secret program associated with the American atomic bomb effort known as the Manhattan Project. The mission was aimed in part at seizing materials, documents, and Italian, French, and German nuclear research scientists in order to keep them from falling into the hands of the Soviet Union. During the operation, a number of leading scientists were captured, including Werner Heisenberg, Otto Hahn, Max von Laue, Kurt Diebner, Walther Gerlach, and Carl Friedrich von Weizsäcker. Kuiper was directly involved in the daring rescue of aging Nobel laureate Max Planck, extracting him from Soviet-occupied territory and delivering him safely to relatives in western Germany.

After World War II ended, Kuiper returned to the United States, where he divided his time between his classes at the University of Chicago and Yerkes Observatory and the McDonald Observatory in Texas. The focus of his investigation shifted from stars to planets as he concentrated on a close examination of the solar system via telescope and spectroscope.

From 1947 to 1949, and then again from 1957 to 1959, Kuiper served as director of both the Yerkes and McDonald Observatories. Throughout his more than twenty years in Chicago, Kuiper headed conferences, edited several important books about the solar system, published a multitude of papers, and made many new discoveries related to the composition and atmosphere of the outer planets that led to new theories of the solar system’s origins. He also inspired such University of Chicago students as Carl Sagan, who would later become a well-known astronomer and author.

In 1960, Kuiper left Chicago for the University of Arizona in Tucson. Soon after his arrival, he organized the Lunar and Planetary Laboratory (LPL), which united segments of the astronomy, geology, and chemistry departments in a comprehensive study of the solar system. The LPL used both the McDonald Observatory and the new Kitt Peak National Observatory in the nearby Quinlan Mountains, which opened in 1958. Kuiper also secured funding to begin constructing a new group of observatories in the neighboring Santa Catalina Mountains and was instrumental in the establishment of observatories in Chile (Cerro Tololo) and on Mauna Kea in Hawaii.

During the 1960s, Kuiper was closely associated with the National Aeronautics and Space Administration (NASA). He was particularly involved with NASA’s Ranger (1961–65), Surveyor (1966–68), and Apollo (1963–72) programs, selecting potential landing sites for the moon-bound spacecraft and editing several lunar atlases and photographic albums that were produced following their successful missions. During the late 1960s and early 1970s, Kuiper pioneered high-altitude astronomy using telescope and infrared-equipped NASA aircraft. He died after suffering a heart attack in Mexico City, Mexico, on December 24, 1973.

Impact

Numerous discoveries in astronomy are forever linked with Kuiper’s name. In the 1930s, he identified several binary stars. In the mid-1940s, while conducting spectroscopic studies of major planets and their satellites, he was first to detect methane on Titan, Saturn’s largest moon and thus far the only moon in the solar system known to have an atmosphere. Several years later, Kuiper found carbon dioxide in the atmosphere of Mars and measured the temperatures and atmospheres of Jupiter and Saturn. In 1948, he spotted Miranda, the smallest of the five main moons of Uranus; in 1949, he identified Nereid, Neptune’s third-largest moon.

In the early 1950s, Kuiper was one of the first scientists to suggest that planetary systems were not a rarity in the universe, as earlier astronomers had supposed, but were in fact commonplace. He speculated that many other stars throughout the galaxies would have planets orbiting about them. The first extra-solar planet, or exoplanet, was not discovered until 1995; since then, dozens of other planets have been detected, proving Kuiper correct. Kuiper also conducted an asteroid survey in the early 1950s, and late in the decade he published photos and data on more than 1,200 such objects. His detailed observations of the solar system, made using infrared spectroscopy, and the multidisciplinary approach he established at the LPL contributed greatly both to NASA’s early successes and to the evolution of astronomy.

Kuiper was recognized often, both during his lifetime and posthumously, for his accomplishments. In 1947, he received the Janssen Medal from the Astronomical Society of France. He was elected a member of the National Academy of Sciences in 1950. The American Astronomical Society awarded him the Henry Norris Russell Lectureship in 1959, and in 1971 he received the prestigious Kepler Gold Medal from the American Association for the Advancement of Science. Since his death, craters on the moon, Mars, and Mercury have been named in his memory. The American Astronomical Society’s Kuiper Prize is annually awarded to leading planetary scientists.

Bibliography

Hall, R. Cargill. Lunar Impact: The NASA History of Project Ranger. Mineola: Dover, 2010. Print. Examines the series of successful American unmanned spacecraft expeditions to the moon, to which Gerard Kuiper was a major contributor. Includes more than one hundred photographs.

Lorenz, Ralph, and Jacqueline Mitton. Lifting Titan’s Veil: Exploring the Giant Moon of Saturn. Cambridge: Cambridge UP, 2002. Print. Presents an illustrated examination of Saturn’s moon Titan, one of the solar system’s largest satellites, which Kuiper discovered to have an Earth-like atmosphere. Includes information about the 2004 Cassini mission to Saturn and the 2005 Huygens probe of Titan.

McBride, Neil, and Iain Gilmour, eds. An Introduction to the Solar System. Cambridge: Cambridge UP, 2004. Print. Covers the evolution of the solar system, with details of all planets, satellites, and other objects found between the sun and the Kuiper belt. Illustrations, photographs, summaries, glossaries of terms.