page_title: Adriana Ocampo
section_title: NASA career
hierarchical_section_title: Adriana Ocampo / NASA career
caption_attribution_description: English: Adriana Ocampo Uria.
context_page_description: Adriana C. Ocampo Uria is a Colombian planetary geologist and a Science Program Manager at NASA Headquarters. In 1970, Ocampo emigrated to California and completed her Master in Sciences at California State University, Northridge and finished her PhD at the Vrije Universiteit in the Netherlands. During high school and graduate studies she worked that the Jet Propulsion Laboratory, where she serves as the lead program executive.
  She and her colleagues were the first to identify a ring of cenotes using satellite images, the only surface impression of the buried Chicxulub crater. This research contributed significantly to the understanding of this impact crater. Ocampo has subsequently led at least seven research expeditions to the Chicxulub site. Ocampo also led the expedition to Belize ejecta site, another crater impact site linked to the Caribbean and Mexico. She continues to search for new impact craters, and with her team, recently reported on a possible crater near Cali, Colombia.
context_section_description: Adriana Ocampo started in 2015 to serve as the lead program executive for the New Frontiers Program at the Jet Propulsion Laboratory. The New Frontiers Program mission is to take the top priorities and goals of the planetary scientific community and address them employing medium-class spacecraft missions that furthers the understanding of the Solar System. These include the Juno mission to Jupiter, the New Horizons mission to Pluto and the asteroid sample return mission OSIRIS-REx. She was also the lead NASA scientist in their collaboration with the European Space Agency's Venus Express mission, and with the Japanese Aerospace Exploration Agency's Venus Climate Orbiter mission. Ocampo has had an asteroid name after her in recognition of her contributions to space exploration. 
  Adriana Ocampo worked in a multi-mission image processing laboratory culminating in a publication in 1980. She was a member of the imaging team for the Viking program were she planned, analyzed, and produced images of Mars' satellites Phobos and Deimos, published by NASA in 1984 and later utilized to plan the Soviet Phobos mission. During this mission the team detected  100 kilometres (62 mi) down through the dense atmosphere of Venus. This was particularly useful to study the "night side" of Venus.  Consequently, the team of scientists constructed the night-side maps of Venus, with resolutions 3 to 6 times better than those of Earth-based telescopes.
  The Chicxulub impact crater is located underneath the Yucatán Peninsula in Mexico. It was hypothesized that this crater was formed by an asteroid leading to mass extinctions on Earth. This was previously postulated in the early 1980s by the physicist Luis Walter Alvarez and his son the geologist Walter Alvarez. However, the only evidence to back this theory was the presence of iridium in the K/T boundary, since this element was found to be mainly present in asteroids and comets. While looking for water resources in Yucatán using satellite images in 1989 and 1990, Ocampo, former NASA archaeologist Kevin O. Pope, and Charles Duller, found cenotes related to this crater. Adriana Ocampo and her colleagues hypothesized that the cenote might be near the impact site, and their findings were later published in Nature in May 1991. In 1991, NASA and The Planetary Society Pasadena sponsored an expedition led by Ocampo and Pope.  During this expedition, Ocampo and her colleges discovered two new sites containing two layers consisting of particles that had been ejected upon impact of the asteroid and then flowed away, generating ejecta lobes. The ejecta lobes at Chicxulub are key to understanding Mars better, since most of that planet is covered by ejecta. Ocampo was awarded her master thesis on the Chicxulub impact crater at California State University.
  
  The Exobiology Program of NASA's Office of Space Science and The Planetary Society of Pasadena sponsored an expedition to the second ejecta site in Belize. Ocampo led expeditions there in January 1995, 1996, and 1998. Small particles resembling green glass, and later identified as tektites, were found at the site. These particles, formed from exposure to high temperatures like the ones generated during the impact, linked this site to other ejecta sites in the Caribbean and Mexico.
  In 2005, Ocampo was a member of the Galileo mission's team . She led of the near-infrared mapping spectrometer (NIMS), on Galileo's project, acting as the science coordinator for flight project mission operations. Galileo was launched in 1989 in route to Jupiter, bearing four remote-sensing instruments, one of them being NIMS. Ocampo was in charge of scheduling the observations of Jupiter's moon Europa, and leading the data analysis. Adriana Ocampo and her colleges published the results of this study in the Icarus journal titled "Galileo's Multiinstrument Spectral View of Europa's Surface Composition". 
  Ocampo led the Juno mission which was in charge of developing strategic plans and recommendations for the research of Jupiter. Juno is the first spacecraft built with solar panels with a
caption: Adriana Ocampo
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