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Lowell Observatory Archives

New Horizons and Current Science

Photograph of Jim Christy holding a glass plate with the Charon discovery image in 1978. 

Discovery images of Pluto's moon, Charon, taken in 1978. 

Artist rendering of the Pluto-Charon sytstem courtesy of the European Organisation for Astronomical Research in the Southern Hemisphere (ESO).

As the 1940s approached, the initial excitement following Pluto’s discovery faded from public interest. War, industrial growth, and international developments all emerged at the forefront of the nation’s mind, leaving Pluto in the shadows once more. The limitations of technology also contributed to the lull in Pluto research between the late 1930s and the 1950s. Scientists had not yet developed machinery powerful enough to endure the long trip from Earth to Pluto, which restricted astronomers to making observations through telescopes and theorizing about the planet’s characteristics. Much like Percival Lowell’s search in the early 1900s, Pluto research during this period was slow and produced little results, but astronomer Gerard Kuiper was eager to learn more about the distant planet. In the late 1940s and 50s, Dr. Kuiper from the Department of Planetary Sciences at the University of Arizona collaborated with fellow astronomer Milton Humason to begin measuring Pluto’s size. They utilized the largest telescope in the world at that time, the Palomar two hundred inch, to observe Pluto by eye. The astronomers soon realized that the planet’s diameter was much smaller than anticipated. Select astronomers across the country began their own observations to validate what Kuiper and Humason proposed and ultimately agreed that Pluto was, indeed, not nearly the size of Earth as Percival Lowell had predicted.

Evidence of Pluto’s new size influenced another small wave of interest in the scientific community throughout the 1960s and 70s. Researchers began studying Pluto’s surface using photoelectric photometry, which measures the brightness of celestial objects such as stars. Other astronomers, like Jim Christy, worked on refining the calculations of Pluto’s orbit around the sun and found much more surprising results. In the spring of 1978, Christy requested images of Pluto from the Naval Observatory Flagstaff Station (NOFS) and on April 13 and May 12 of that year, astronomer Anthony Hewitt took the requested photographs on glass plates before sending them to Christy in Washington, D.C. Christy began studying the plates on June 22, 1978 and found an abnormal bulge that seemed to protrude from Pluto. After studying images of Pluto and the movement of that abnormality, Christy realized that the image had captured Pluto’s moon. In the upper left corner, the discovery plate of Pluto’s moon is featured. The left panel shows an elongated Pluto, not quite circular because its moon is peeking over the top of the planet. The right panel shows a perfectly circular Pluto lined up with its moon. With assistance from a colleague, Christy began calculating the orbit of the moon and determining its name. He took his wife’s nickname, “Char,” and added “-on” like the ending of “proton” and “electron,” but he feared that using the name “Charon” would not follow the trend of naming celestial objects after characters from mythology. To his surprise, Christy found that the name “Charon” was also the name of the ferryman in Roman mythology who transported souls across the River Styx into the underworld, which is ruled by the god Pluto. Below the plate image is an artist’s rendering of Pluto and its moon, Charon.

The discovery of Charon raised even more questions and inspired further interest in Pluto research. Researchers continued to study images of Pluto and Charon, but technological developments in the 1990s propelled Pluto studies further than it had ever gone. Astronomers Alan Stern and Marc Buie were especially interested in using the newly developed Hubble Space telescope to further explore Pluto’s surface. Hubble technology confirmed several theories about the Pluto system, including the fact that Charon is tidally locked meaning that it only shows one face as it rotates about Pluto. Thanks to Hubble, astronomers were also able to study the Pluto system’s surface and atmosphere using infrared wavelengths, which showed them the various gasses found on both Pluto and Charon. 

Audio clip from an interview between Dr. Will Grundy and Lowell Observatory's archives intern, Melissa Valenzuela. Conducted in 2022 seven years after NASA's New Horizons mission, Dr. Grundy explains the significant outcomes of the expedition and its impact on current planetary research.

New Horizons and Current Science