Alberto Conti | |
---|---|
Born | Palmanova, Italy | September 27, 1966
Nationality | Italian, American |
Alma mater | Ohio State University |
Known for | GoogleSky (Sky in Google Earth) |
Awards | Outstanding Science & Technology Emmy Award Pirelli Internetional Award |
Scientific career | |
Fields | Astrophysics |
Institutions | BAE Systems Inc. |
Doctoral advisor | Barbara Ryden Patrick Osmer David Weinberg |
Alberto Conti (born September 27, 1966), is an astrophysicist and the Vice President and General Manager of the Civil Space Strategic Business Unit (SBU) at BAE Systems Inc.. He is one of the creators of the GoogleSky concept, of the idea of astronomical outreach at South by SouthWest 2013 and of the James Webb Space Telescope iBook. He is also the Executive Producer of the Emmy Winning CNN Films The Hunt for Planet B.
Conti was born in Palmanova, Italy. He received his laurea degree in physics from the University of Trieste, Italy, with a thesis titled "Binary Galaxies in the Center for Astrophysics | Harvard & Smithsonian (CfA) Redshift Survey." During the following two years, he worked on the largest sample (at the time) of optical rotation curves of galaxies at the International School for Advanced Studies (SISSA), in Trieste. There he developed algorithms to automate the extraction of physical parameters from galactic rotation curves, paving the way for the analysis of much larger samples. He has since specialized in statistical methods, computational astrophysics, and large datasets.
in 2000 Conti graduated from the Ohio State University with a Ph.D. thesis on correlating galactic properties with the physics of galaxy formation. [1] He then became a postdoctoral researcher at the Department of Physics and Astronomy of the University of Pittsburgh where he focused on the star formation history of galaxies. [2]
In 2003, Conti joined the Space Telescope Science Institute (STScI) to co-lead the development of a new archive for the Galaxy Evolution Explorer (GALEX [3] ). He integrated this effort with work on the National Virtual Observatory.
In January 2005, he became Branch Manager for the Astronomy Tools and Applications (ASTTA) branch at STScI's Engineering System and Software Division. ASTTA develops some of the best-known software products for the astronomical community, such as Astronomer Proposal Tool, PyRAF, and Multidrizzle.
At the 15th annual ADASS conference in October 2005, Conti became interested in the Google Earth software that allows anyone to browse Earth with a simple point-and-click interface. Back at STScI he sent a proposal to John Hanke, the Head of Google Earth and Google Maps, to extend the Google Earth interface to space-based data. Hanke agreed to have Brian McClendon establish a project plan for such a product, called GoogleSky. [4]
In September 2006, Conti became Chief Engineer for the Data Management System at STScI. Following his involvement with Google he became Development Manager at STScI's Community Missions Office (CMO). CMO serves as the conduit between mission teams and STScI personnel to ensure support for mission science operations, data archiving, grants administration, peer review and education/outreach.
In 2008 Conti received first prize in the Pirelli Internetional Award for the development of GoogleSky. [5]
In 2010, Conti became the Archive Scientist for the Multimission Archive at Space Telescope, the NASA UV and Optical data archive.
In 2011, Conti became the Innovation Scientist for the James Webb Space Telescope, NASA's premier space observatory of the next decade.
In 2013, Conti became the Innovation Manager for the Civil Air and Space at Northrop Grumman Corporation.
In 2018, Conti became the Director for New Business and Innovative Solutions at Ball Aerospace & Technologies.
In 2022, Conti was honored with an Emmy by the National Academy of Television Arts and Sciences (NATAS) as an Executive Producer of the CNN Films The Hunt for Planet B. Directed by Nathaniel Khan, The Hunt for Planet B is a human drama behind NASA's high-stakes James Webb Space Telescope which launched on December 25, 2021. [6] In this same year, he was promoted to vice president and General Manager for the Civil Space Strategic Business Unit at Ball Aerospace & Technologies [7]
The following outline is provided as an overview and topical guide to space science:
The Hubble Space Telescope is a space telescope that was launched into low Earth orbit in 1990 and remains in operation. It was not the first space telescope, but it is one of the largest and most versatile, renowned as a vital research tool and as a public relations boon for astronomy. The Hubble telescope is named after astronomer Edwin Hubble and is one of NASA's Great Observatories. The Space Telescope Science Institute (STScI) selects Hubble's targets and processes the resulting data, while the Goddard Space Flight Center (GSFC) controls the spacecraft.
The Space Telescope Science Institute (STScI) is the science operations center for the Hubble Space Telescope (HST), science operations and mission operations center for the James Webb Space Telescope (JWST), and science operations center for the Nancy Grace Roman Space Telescope. STScI was established in 1981 as a community-based science center that is operated for NASA by the Association of Universities for Research in Astronomy (AURA). STScI's offices are located on the Johns Hopkins University Homewood Campus and in the Rotunda building in Baltimore, Maryland.
The James Webb Space Telescope (JWST) is a space telescope designed to conduct infrared astronomy. As the largest telescope in space, it is equipped with high-resolution and high-sensitivity instruments, allowing it to view objects too old, distant, or faint for the Hubble Space Telescope. This enables investigations across many fields of astronomy and cosmology, such as observation of the first stars and the formation of the first galaxies, and detailed atmospheric characterization of potentially habitable exoplanets.
Galaxy Evolution Explorer was a NASA orbiting space telescope designed to observe the universe in ultraviolet wavelengths to measure the history of star formation in the universe. In addition to paving the way for future ultraviolet missions, the space telescope allowed astronomers to uncover mysteries about the early universe and how it evolved, as well as better characterize phenomena like black holes and dark matter. The mission was extended three times over a period of 10 years before it was decommissioned in June 2013. GALEX was launched on 28 April 2003 and decommissioned in June 2013.
Stephan's Quintet is a visual grouping of five galaxies of which four form the first compact galaxy group ever discovered. The group, visible in the constellation Pegasus, was discovered by Édouard Stephan in 1877 at the Marseille Observatory. The group is the most studied of all the compact galaxy groups. The brightest member of the visual grouping is NGC 7320, which has extensive H II regions, identified as red blobs, where active star formation is occurring.
Messier 21 or M21, also designated NGC 6531 or Webb's Cross, is an open cluster of stars located to the north-east of Sagittarius in the night sky, close to the Messier objects M20 to M25. It was discovered and catalogued by Charles Messier on June 5, 1764. This cluster is relatively young and tightly packed. A few blue giant stars have been identified in the cluster, but Messier 21 is composed mainly of small dim stars. With a magnitude of 6.5, M21 is not visible to the naked eye; however, with the smallest binoculars it can be easily spotted on a dark night. The cluster is positioned near the Trifid nebula, but is not associated with that nebulosity. It forms part of the Sagittarius OB1 association.
Messier 63 or M63, also known as NGC 5055 or the seldom-used Sunflower Galaxy, is a spiral galaxy in the northern constellation of Canes Venatici with approximately 400 billion stars. M63 was first discovered by the French astronomer Pierre Méchain, then later verified by his colleague Charles Messier on 14 June 1779. The galaxy became listed as object 63 in the Messier Catalogue. In the mid-19th century, Anglo-Irish astronomer Lord Rosse identified spiral structures within the galaxy, making this one of the first galaxies in which such structure was identified.
The Digitized Sky Survey (DSS) is a digitized version of several photographic astronomical surveys of the night sky, produced by the Space Telescope Science Institute between 1983 and 2006.
The Sculptor Galaxy is an intermediate spiral galaxy in the constellation Sculptor. The Sculptor Galaxy is a starburst galaxy, which means that it is currently undergoing a period of intense star formation.
HD 80606 and HD 80607 are two stars comprising a binary star system. They are approximately 217 light-years away in the constellation of Ursa Major. Both stars orbit each other at an average distance of 1,200 astronomical units. The binary system is listed as Struve 1341 in the Struve Catalogue of Double Stars; however, this designation is not in wide use and the system is usually referred to by the HD designations of its constituent stars. An extrasolar planet has been confirmed to orbit HD 80606 in a highly elliptical orbit.
NGC 1566, sometimes known as the Spanish Dancer, is an intermediate spiral galaxy in the constellation Dorado, positioned about 3.5° to the south of the star Gamma Doradus. It was discovered on May 28, 1826 by Scottish astronomer James Dunlop. At 10th magnitude, it requires a telescope to view. The distance to this galaxy remains elusive, with measurements ranging from 6 Mpc up to 21 Mpc.
Charles Mattias ("Matt") Mountain is currently the President of the Association of Universities for Research in Astronomy (AURA) which designs, builds, and operates telescopes and observatories for the National Science Foundation (NSF) and the National Aeronautics and Space Administration (NASA). AURA's NASA center is the Space Telescope Science Institute (STScI), responsible for the science mission for the Hubble Space Telescope, the science and operations for the James Webb Space Telescope, and the MAST data archive. AURA's NSF centers are Gemini Observatory, the National Optical Astronomy Observatory (NOAO), and the National Solar Observatory (NSO). Dr. Mountain and AURA are also responsible for the NSF construction projects: the Daniel K. Inouye Solar Telescope (DKIST) on Haleakalā, Hawaii and the Large Synoptic Survey Telescope (LSST) on Cerro Pachón in Chile.
The Large Ultraviolet Optical Infrared Surveyor, commonly known as LUVOIR, is a multi-wavelength space telescope concept being developed by NASA under the leadership of a Science and Technology Definition Team. It is one of four large astrophysics space mission concepts studied in preparation for the National Academy of Sciences 2020 Astronomy and Astrophysics Decadal Survey.
NGC 3642 is a spiral galaxy in the constellation Ursa Major. The galaxy has a low-ionization nuclear emission-line region. It is located at a distance of circa 30 million light years from Earth, which, given its apparent dimensions, means that NGC 3642 is about 50,000 light years across. The galaxy is characterised by an outer pseudoring, which was probably formed after the accretion of a gas rich dwarf galaxy.
The Mikulski Archive for Space Telescopes (MAST) is an astronomical data archive. The archive brings together data from the visible, ultraviolet, and near-infrared wavelength regimes. The NASA funded project is located at the Space Telescope Science Institute (STScI) in Baltimore, Maryland and is one of the largest astronomical databases in the world.
NGC 2336 is a barred spiral galaxy located in the constellation Camelopardalis. It is located at a distance of circa 100 million light years from Earth, which, given its apparent dimensions, means that NGC 2336 is about 200,000 light years across. It was discovered by Wilhelm Tempel in 1876.
NGC 5965 is a spiral galaxy located in the constellation Draco. It is located at a distance of circa 150 million light years from Earth, which, given its apparent dimensions, means that NGC 5965 is about 260,000 light years across. It was discovered by William Herschel on May 5, 1788.
NGC 2525 is a barred spiral galaxy located in the constellation Puppis. It is located at a distance of about 70 million light years from Earth, which, given its apparent dimensions, means that NGC 2525 is about 60,000 light years across. It was discovered by William Herschel on February 23, 1791.