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  • USA_SCI_RT_03_xs .Photo illustration:.Radio Telescope: The Mars Antenna in the Mojave Desert, California the Goldstone Deep Space Communications Complex with 6 exposures of the eclipse of the moon. Standing 24 stories tall, the Mars antenna is the largest dish at Goldstone. It was originally built as a 64-meter-diameter (210-foot) antenna and received its first signal from the Mariner 4 mission to Mars. By 1988, the Mars dish, along with the 64-meter antennas in Spain and Australia, was upgraded to 70 meters (230 feet). These 70-meter antennas increase the receiving power of the Deep Space Network. (1983)
    USA_SCI_RT_03_xs.jpg
  • Radio Telescope: The Mars Antenna in the Mojave Desert, California. Goldstone Deep Space Communications Complex. Standing 24 stories tall, the Mars antenna is the largest dish at Goldstone. It was originally built as a 64-meter-diameter (210-foot) antenna and received its first signal from the Mariner 4 mission to Mars. By 1988, the Mars dish, along with the 64-meter antennas in Spain and Australia, was upgraded to 70 meters (230 feet). These 70-meter antennas increase the receiving power of the Deep Space Network. (1983)
    USA_SCI_RT_01_xs.jpg
  • Radio Telescope: The Mars Antenna in the Mojave Desert, California. Goldstone Deep Space Communications Complex. Standing 24 stories tall, the Mars antenna is the largest dish at Goldstone. It was originally built as a 64-meter-diameter (210-foot) antenna and received its first signal from the Mariner 4 mission to Mars. By 1988, the Mars dish, along with the 64-meter antennas in Spain and Australia, was upgraded to 70 meters (230 feet). These 70-meter antennas increase the receiving power of the Deep Space Network. Time exposure shows the rotation of the earth (the light from stars are recorded as curved steaks). (1983)
    USA_SCI_RT_02_xs.jpg
  • Radio Telescope: The Mars Antenna in the Mojave Desert, California. Goldstone Deep Space Communications Complex. Standing 24 stories tall, the Mars antenna is the largest dish at Goldstone. It was originally built as a 64-meter-diameter (210-foot) antenna and received its first signal from the Mariner 4 mission to Mars. By 1988, the Mars dish, along with the 64-meter antennas in Spain and Australia, was upgraded to 70 meters (230 feet). These 70-meter antennas increase the receiving power of the Deep Space Network. (1983)
    USA_SCI_RT_04_xs.jpg
  • Radio Telescope: The Mars Antenna in the Mojave Desert, California. Goldstone Deep Space Communications Complex. Standing 24 stories tall, the Mars antenna is the largest dish at Goldstone. It was originally built as a 64-meter-diameter (210-foot) antenna and received its first signal from the Mariner 4 mission to Mars. By 1988, the Mars dish, along with the 64-meter antennas in Spain and Australia, was upgraded to 70 meters (230 feet). These 70-meter antennas increase the receiving power of the Deep Space Network. (1983)
    USA_SCI_RT_05_xs.jpg
  • Parkes radio telescope. The huge dish of the radio telescope at the Australian National Radio Astronomy Observatory at Parkes, New South Wales, Australia. The dish is 64 meters (210 feet) in diameter and is fully steer-able. It was completed in 1961, and can be used to record a range of wavelengths from 5 millimeters to 2 centimeters. (1989)
    AUS_SCI_RT_02_xs.jpg
  • Engineers on a radio antenna under construction with rainbow on the distance. The Very Long Baseline Array (VLBA) is a system of 10 radio telescopes controlled remotely from the Array Operations Center in Socorro, New Mexico. The antennas are spread across the United States from St. Croix in the Virgin Islands to Mauna Kea on the island of Hawaii, making it the world's largest dedicated, full-time astronomical instrument..This antenna at Pie Town, New Mexico, is now linked with the Very Large Array via fiber optics. It is the first part of the planned Expanded Very Large Array...(1988)
    USA_SCI_RT_15_xs.jpg
  • Radio Telescope: The Mars Antenna in the Mojave Desert, California. Goldstone Deep Space Communications Complex. Standing 24 stories tall, the Mars antenna is the largest dish at Goldstone. It was originally built as a 64-meter-diameter (210-foot) antenna and received its first signal from the Mariner 4 mission to Mars. By 1988, the Mars dish, along with the 64-meter antennas in Spain and Australia, was upgraded to 70 meters (230 feet). These 70-meter antennas increase the receiving power of the Deep Space Network. (1983)
    USA_SCI_RT_06_xs.jpg
  • Parkes radio telescope. The huge dish of the radio telescope at the Australian National Radio Astronomy Observatory at Parkes, New South Wales, Australia. The dish is 64 meters (210 feet) in diameter and is fully steer-able. It was completed in 1961, and can be used to record a range of wavelengths from 5 millimeters to 2 centimeters. (1989)
    AUS_SCI_RT_01_xs.jpg
  • Radio Telescopes. Near Stanford University, Palo Alto, California. (1997)
    USA_SCI_RT_12_xs.jpg
  • Jill Tarter. Portrait of Jill Tarter (1944-), American astrophysicist and SETI researcher with a radiotelescope at Stanford, CA. Palo Alto, California. MODEL RELEASED (1988)
    USA_SCI_RT_13_xs.jpg
  • Jill Tarter. Portrait of Jill Tarter (1944-), American astrophysicist and SETI researcher with a princess phone at a radiotelescope at Stanford, CA. Palo Alto, California. (1988)
    USA_SCI_RT_14_xs.jpg
  • View of some of the dish antennae which make up the Very Large Array (VLA) radio telescope near Socorro, New Mexico. The VLA is the world's largest radio telescope array, consisting of 27 dish antennae, each one 25 meters in diameter. The dishes can be moved to various positions along the arms of a Y-shaped railway network; two of these railway arms are 21 km in length, the third 19 km. The data obtained by the dishes are combined by computer to form a single radio image, so that the 27 antennae in effect form one single giant radio dish. (1984)
    USA_SCI_RT_11_xs.jpg
  • View of some of the dish antennae which make up the Very Large Array (VLA) radio telescope near Socorro, New Mexico. The VLA is the world's largest radio telescope array, consisting of 27 dish antennae, each one 25 meters in diameter. The dishes can be moved to various positions along the arms of a Y-shaped railway network; two of these railway arms are 21 km in length, the third 19 km. The data obtained by the dishes are combined by computer to form a single radio image, so that the 27 antennae in effect form one single giant radio dish. (1984)
    USA_SCI_RT_09_xs.jpg
  • View of some of the dish antennae which make up the Very Large Array (VLA) radio telescope near Socorro, New Mexico. The VLA is the world's largest radio telescope array, consisting of 27 dish antennae, each one 25 meters in diameter. The dishes can be moved to various positions along the arms of a Y-shaped railway network; two of these railway arms are 21 km in length, the third 19 km. The data obtained by the dishes are combined by computer to form a single radio image, so that the 27 antennae in effect form one single giant radio dish. (1984)
    USA_SCI_RT_10_xs.jpg
  • View of some of the dish antennae which make up the Very Large Array (VLA) radio telescope near Socorro, New Mexico. The VLA is the world's largest radio telescope array, consisting of 27 dish antennae, each one 25 meters in diameter. The dishes can be moved to various positions along the arms of a Y-shaped railway network; two of these railway arms are 21 km in length, the third 19 km. The data obtained by the dishes are combined by computer to form a single radio image, so that the 27 antennae in effect form one single giant radio dish. (1984)
    USA_SCI_RT_08_xs.jpg
  • View of some of the dish antennae which make up the Very Large Array (VLA) radio telescope near Socorro, New Mexico. The VLA is the world's largest radio telescope array, consisting of 27 dish antennae, each one 25 meters in diameter. The dishes can be moved to various positions along the arms of a Y-shaped railway network; two of these railway arms are 21 km in length, the third 19 km. The data obtained by the dishes are combined by computer to form a single radio image, so that the 27 antennae in effect form one single giant radio dish. (1984).
    USA_SCI_RT_07_xs.jpg
  • Inside the control room of a 25-meter diameter dish which makes up the Very Large Array (VLA) radio telescope near Socorro, New Mexico. The VLA is the world's largest radio telescope array, consisting of 27 dish antennae, each one 25 meters in diameter. The dishes can be moved to various positions along the arms of a Y-shaped railway network; two of these railway arms are 21 km in length, the third 19 km. The data obtained by the dishes are combined by computer to form a single radio image, so that the 27 antennae in effect form one single giant radio dish. (1984). Radio Telescope. Los Alamos, New Mexico. (1988)
    USA_SCI_RT_16_xs.jpg
  • Lick Observatory. Time exposure image showing star trails over a telescope dome at the Lick Observatory on Mount Hamilton in California, USA. In the foreground are trails from red taillights of a car. Astronomers often carry red flashlights so that their night vision is not affected. Completed in 1888 at an altitude of 1280 meters, Lick was the world's first permanent mountaintop observatory. Its location provided excellent viewing conditions for years until light pollution from the nearby city of San Jose began to interfere with results. In 1997 the observatory is operated by California University. Star trails are caused by what seems to be the motion of the stars due to the rotation of the Earth about its axis.
    USA_SCI_ASTR_01_120_xs.jpg
  • Lick Observatory. Time exposure image showing star trails over a telescope dome at the Lick Observatory on Mount Hamilton in California, USA. In the foreground are trails from red flashlights carried by astronomers so that their night vision is not affected. Completed in 1888 at an altitude of 1280 meters, Lick was the world's first permanent mountaintop observatory. Its location provided excellent viewing conditions for years until light pollution from the nearby city of San Jose began to interfere with results. In 1997 the observatory is operated by California University. Star trails are caused by what seems to be the motion of the stars due to the rotation of the Earth about its axis. (1996)
    USA_SCI_ASTR_01_xs.jpg
  • Mountain View, California.David Koch, a researcher at the NASA/Ames Research Center in Mountain View, California, displays an area in the sky that can be approximated by two handfuls of sky at arms length. David Koch is planning to search an area of this size with the KEPLER space telescope/photometer for as of yet undiscovered terrestrial planets in the "habitable zone". The area he plans to study is located in the Milky Way, and is known as the H-2 area. Koch plans to search this area using the KEPLER orbiting telescope, looking at 100,000 stars every four minutes for four years. In doing so, he expects to find about 400 earth sized planets as well as 800 planets twice the size of earth. Koch is double exposed with the 120 inch telescope at the Lick Observatory on Mt. Hamilton and the night sky. MODEL RELEASED [1999]
    USA_SCI_NASA_10_xs.jpg
  • Lick Observatory on Mt. Hamilton. San Jose, California. 120-inch telescope.  Exoplanets & Planet Hunters
    USA_Lick_060513_174_rwx.jpg
  • Lick Observatory on Mt. Hamilton. San Jose, California. 120-inch telescope.  Exoplanets & Planet Hunters
    USA_Lick_060513_179_rwx.jpg
  • Lick Observatory on Mt. Hamilton. San Jose, California. 120-inch telescope.  Exoplanets & Planet Hunters
    USA_Lick_060513_176_rwx.jpg
  • View of San Jose and Silicon Valley from the Lick Observatory on Mt. Hamilton. San Jose, California.
    USA_Lick_060513_169_rwx.jpg
  • Lick Observatory on Mt. Hamilton. San Jose, California. 120-inch telescope.
    USA_Lick_060513_159_rwx.jpg
  • Lick Observatory on Mt. Hamilton. San Jose, California. Old computer equipment put out for recycling/trash pickup. Outside the 120-inch telescope. (Dome is lit by the full moon, 30-second exposure.)  Exoplanets & Planet Hunters
    USA_Lick_060513_195_rwx.jpg
  • Lick Observatory on Mt. Hamilton. San Jose, California. Old computer equipment put out for recycling/trash pickup. Outside the 120-inch telescope. (Dome is lit by the full moon, 30-second exposure.)  Exoplanets & Planet Hunters
    USA_Lick_060513_194_rwx.jpg
  • Lick Observatory on Mt. Hamilton. San Jose, California. Old computer equipment put out for recycling/trash pickup. Outside the 120-inch telescope. (Dome is lit by the full moon, 30-second exposure.)  Exoplanets & Planet Hunters
    USA_Lick_060513_201_rwx.jpg
  • Lick Observatory on Mt. Hamilton. San Jose, California. 120-inch telescope. Chris McCarthy, astronomer.  Exoplanets & Planet Hunters
    USA_Lick_060513_048_rwx.jpg
  • Lick Observatory on Mt. Hamilton. San Jose, California. 120-inch telescope.
    USA_Lick_060513_110_rwx.jpg
  • Lick Observatory on Mt. Hamilton. San Jose, California. Chris McCarthy, astronomer, with the 120-inch telescope.
    USA_Lick_060513_263_rwx.jpg
  • Lick Observatory on Mt. Hamilton. San Jose, California. Chris McCarthy, astronomer, with the 120-inch telescope
    USA_Lick_060513_259_rwx.jpg
  • .COMPOSITE PHOTO. Lick Observatory on Mt. Hamilton. San Jose, California. Chris McCarthy, astronomer, with the 120-inch telescope. THIS IMAGE COMBINES TWO DIFFERENT EXPOSURES OF THE TELESCOPE AND DOME IN THE BACKGROUND. SEE 268 AND 263 FOR ORIGINAL IMAGES.  Exoplanets & Planet Hunters
    USA_Lickcomb_060513_263_rwx.jpg
  • Lick Observatory on Mt. Hamilton. San Jose, California. 120-inch telescope.  Exoplanets & Planet Hunters
    USA_Lick_060513_268_rwx.jpg
  • .COMPOSITE PHOTO. Lick Observatory on Mt. Hamilton. San Jose, California. Chris McCarthy, astronomer, with the 120-inch telescope. THIS IMAGE COMBINES TWO DIFFERENT EXPOSURES OF THE TELESCOPE AND DOME IN THE BACKGROUND. SEE 263 AND 268 FOR ORIGINAL IMAGES.  Exoplanets & Planet Hunters
    USA_Lickcomb_060513_263_268_rwx.jpg
  • Lick Observatory on Mt. Hamilton. San Jose, California. 120-inch telescope. Chris McCarthy, astronomer.  Exoplanets & Planet Hunters
    USA_Lick_060513_079_rwx.jpg
  • Lick Observatory on Mt. Hamilton. San Jose, California. 120-inch telescope. Chris McCarthy, astronomer.  Exoplanets & Planet Hunters
    USA_Lick_060513_072_rwx.jpg
  • Chris McCarthy, astronomer, having his dinner in the dining hall of the Lick Observatory on Mt. Hamilton. San Jose, California. Chris stays at the observatory for 4 nights in a row. The cook, Dennise Casey, makes him a 'night lunch' (in paper bag) every evening since he works all night at the 120-inch telescope. His night lunch consists of 2 sandwiches, fruit, potato or corn chips and 3 cookies. Chris is a vegetarian.  Exoplanets & Planet Hunters
    USA_Lick_060513_103_rwx.jpg
  • Chris McCarthy, astronomer, having his dinner in the dining hall of the Lick Observatory on Mt. Hamilton. San Jose, California. Chris stays at the observatory for 4 nights in a row. The cook, Dennise Casey, makes him a 'night lunch' (in paper bag) every evening since he works all night at the 120-inch telescope. His night lunch consists of 2 sandwiches, fruit, potato or corn chips and 3 cookies. Chris is a vegetarian.  Exoplanets & Planet Hunters
    USA_Lick_060513_094_rwx.jpg
  • Chris McCarthy, astronomer, having his dinner in the dining hall of the Lick Observatory on Mt. Hamilton. San Jose, California. Chris stays at the observatory for 4 nights in a row. The cook, Dennise Casey, makes him a 'night lunch' (in paper bag) every evening since he works all night at the 120-inch telescope. His night lunch consists of 2 sandwiches, fruit, potato or corn chips and 3 cookies. Chris is a vegetarian.  Exoplanets & Planet Hunters
    USA_Lick_060513_087_rwx.jpg
  • Chris McCarthy, astronomer, having his dinner in the dining hall of the Lick Observatory on Mt. Hamilton. San Jose, California. Chris stays at the observatory for 4 nights in a row. The cook, Dennise Casey, makes him a 'night lunch' (in paper bag) every evening since he works all night at the 120-inch telescope. His night lunch consists of 2 sandwiches, fruit, potato or corn chips and 3 cookies. Chris is a vegetarian.  Exoplanets & Planet Hunters
    USA_Lick_060513_107_rwx.jpg
  • Chris McCarthy, astronomer, having his dinner in the dining hall of the Lick Observatory on Mt. Hamilton. San Jose, California. Chris stays at the observatory for 4 nights in a row. The cook, Dennise Casey, makes him a 'night lunch' (in paper bag) every evening since he works all night at the 120-inch telescope. His night lunch consists of 2 sandwiches, fruit, potato or corn chips and 3 cookies. Chris is a vegetarian.  Exoplanets & Planet Hunters
    USA_Lick_060513_022_rwx.jpg
  • Lick Observatory on Mt. Hamilton. San Jose, California. 120-inch telescope. Telescope operator, Bernie Walp, aims the 120-inch telescope at star HR3982, Rugulus, the brightest star in the Constellation Leo.
    USA_Lick_060513_228_rwx.jpg
  • Lick Observatory on Mt. Hamilton. San Jose, California. 120-inch telescope. Telescope operator, Bernie Walp, aims the 120-inch telescope at star HR3982, Rugulus, the brightest star in the Constellation Leo.  Exoplanets & Planet Hunters
    USA_Lick_060513_237_rwx.jpg
  • This is the "iodine cell," a device developed and perfected by Butler, Marcy, and instrument specialist Steven Vogt of the University of California, Santa Cruz. When light from a star passes through the iodine, molecules in the hot vapor absorb parts of the light at very specific energies. Then, a specially etched slab of glass spreads the starlight into a glorious rainbow spectrum?like a prism held up to the sun, but with exquisitely fine detail. Because the iodine has subtracted bits of the light, a forest of dark black lines covers the spectrum like a long supermarket bar code. "It's like holding the star up to a piece of graph paper," McCarthy says. "The iodine lines never move. So if the star moves, we use the iodine lines as a ruler against which to measure that motion."  Iodine cell.  Lick Observatory on Mt. Hamilton. San Jose, California. 120-inch telescope. Exoplanets & Planet Hunters.
    USA_Lick_060513_032_B_rwx.jpg
  • This is the "iodine cell," a device developed and perfected by Butler, Marcy, and instrument specialist Steven Vogt of the University of California, Santa Cruz. When light from a star passes through the iodine, molecules in the hot vapor absorb parts of the light at very specific energies. Then, a specially etched slab of glass spreads the starlight into a glorious rainbow spectrum?like a prism held up to the sun, but with exquisitely fine detail. Because the iodine has subtracted bits of the light, a forest of dark black lines covers the spectrum like a long supermarket bar code. "It's like holding the star up to a piece of graph paper," McCarthy says. "The iodine lines never move. So if the star moves, we use the iodine lines as a ruler against which to measure that motion."  Iodine cell.  Lick Observatory on Mt. Hamilton. San Jose, California. 120-inch telescope. Exoplanets & Planet Hunters.
    USA_Lick_060513_031_rwx.jpg
  • Lick Observatory. Telescope dome at sunset at the Lick Observatory on Mount Hamilton in California, USA. Completed in 1888 at an altitude of 1280 meters, the Lick Observatory was the world's first permanent mountaintop observatory. Its location provided excellent viewing conditions for years until light pollution from the nearby city of San Jose began to interfere with results. In 1997 the observatory is operated by California University. (1999)
    USA_SCI_ASTR_04_xs.jpg
  • Lick Observatory on Mt. Hamilton. San Jose, California.  Computer screen during Chris McCarthy's night long search for other planets. This shows the spectrum of a start (eschelle spectrum) from 61 Virginis. Spectral lines will move if the star has a planet?this is the motion that they are trying to detect. The sensitivity needs to read 1/1000 of a pixel. 120-inch telescope.  Exoplanets & Planet Hunters
    USA_Lick_060513_247_rwx.jpg
  • Lick Observatory on Mt. Hamilton. San Jose, California. Old computer equipment put out for recycling/trash pickup. Outside the 120-inch telescope. (Dome is lit by the full moon, 30-second exposure.)  Exoplanets & Planet Hunters
    USA_Lick_060513_205_rwx.jpg
  • Lick Observatory on Mt. Hamilton. San Jose, California. 120-inch telescope. Telescope operator, Bernie Walp, aims the 120-inch telescope at star HR3982, Rugulus, the brightest star in the Constellation Leo.
    USA_Lick_060513_239_rwx.jpg
  • Astronomer Geoff Marcy above the lights of the UC Berkeley Campus surrounded by light trails representing swooping eccentric orbits of exoplanets. Unlike the planets of our solar system, the orbits of most of the exoplanets Marcy and his team have discovered are squashed into shapes more like ovals, footballs, and cigars.
    USA_060516_040_rwx.jpg
  • Astronomer Geoff Marcy above the lights of the UC Berkeley Campus surrounded by light trails representing swooping eccentric orbits of exoplanets. Unlike the planets of our solar system, the orbits of most of the exoplanets Marcy and his team have discovered are squashed into shapes more like ovals, footballs, and cigars.
    USA_060516_044_rwx.jpg
  • Astronomer Geoff Marcy above the lights of the UC Berkeley Campus surrounded by light trails representing swooping eccentric orbits of exoplanets. Unlike the planets of our solar system, the orbits of most of the exoplanets Marcy and his team have discovered are squashed into shapes more like ovals, footballs, and cigars.
    USA_060516_037_xrw.jpg
  • Astronomer Geoff Marcy above the lights of the UC Berkeley Campus surrounded by light trails representing swooping eccentric orbits of exoplanets. Unlike the planets of our solar system, the orbits of most of the exoplanets Marcy and his team have discovered are squashed into shapes more like ovals, footballs, and cigars.
    USA_060516_032_xrw.jpg
  • Berkeley and Oakland below the Lawrence Hall of Science with San Francisco in the distance.
    USA_060516_045_rwx.jpg
  • The roof of Cambell Hall at UC Berkeley (California) with a 14 inch telescope in the foreground.  Exoplanets & Planet Hunters
    USA_060516_158_rwx.jpg
  • Astronomer Geoff Marcy on the roof of Cambell Hall at UC Berkeley (California) with 14 inch telescopes. Marcy and his team have detected a large number of exoplanets using data collected from large telescopes at other sites.  Exoplanets & Planet Hunters
    USA_060516_175_rwx.jpg
  • Astronomer Geoff Marcy on the roof of Cambell Hall at UC Berkeley (California) with 14 inch telescopes. Marcy and his team have detected a large number of exoplanets using data collected from large telescopes at other sites.  Exoplanets & Planet Hunters
    USA_060516_107_rwx.jpg
  • Astronomer Geoff Marcy on the roof of Cambell Hall at UC Berkeley (California) with 14 inch telescopes. Marcy and his team have detected a large number of exoplanets using data collected from large telescopes at other sites.  Exoplanets & Planet Hunters
    USA_060516_135_rwx.jpg
  • The roof of Cambell Hall at UC Berkeley (California) with a 14 inch telescope. The University Campanile is in the background. Geoff Marcy and his team have detected a large number of exoplanets using data collected from large telescopes at other sites.  Exoplanets & Planet Hunters
    USA_060516_122_rwx.jpg
  • Astronomer Geoff Marcy on the roof of Cambell Hall at UC Berkeley (California) with 14 inch telescopes. Marcy and his team have detected a large number of exoplanets using data collected from large telescopes at other sites.  Exoplanets & Planet Hunters
    USA_060516_165_rwx.jpg
  • In his UC Berkeley, CA office, astronomer Geoff Marcy is discussing the effects of Einstein's theory of relativity in the measurements of the Doppler shift that allow his team to detect planets.   They make all of their observations from the Earth that moves so fast in its orbit around the Sun that they must include the theory of relativity in their calculations. Exoplanets & Planet Hunters.
    USA_060516_080_rwx.jpg
  • In his UC Berkeley, CA office, astronomer Geoff Marcy is discussing the effects of Einstein's theory of relativity in the measurements of the Doppler shift that allow his team to detect planets.   They make all of their observations from the Earth that moves so fast in its orbit around the Sun that they must include the theory of relativity in their calculations. Exoplanets & Planet Hunters.
    USA_060516_072_rwx.jpg
  • In his UC Berkeley, CA office, astronomer Geoff Marcy is discussing the effects of Einstein's theory of relativity in the measurements of the Doppler shift that allow his team to detect planets.   They make all of their observations from the Earth that moves so fast in its orbit around the Sun that they must include the theory of relativity in their calculations. Exoplanets & Planet Hunters.
    USA_060516_082_rwx.jpg
  • In his UC Berkeley, CA office, astronomer Geoff Marcy is discussing the effects of Einstein's theory of relativity in the measurements of the Doppler shift that allow his team to detect planets.   They make all of their observations from the Earth that moves so fast in its orbit around the Sun that they must include the theory of relativity in their calculations. Exoplanets & Planet Hunters.
    USA_060516_092_rwx.jpg
  • In his UC Berkeley, CA office, astronomer Geoff Marcy is discussing the effects of Einstein's theory of relativity in the measurements of the Doppler shift that allow his team to detect planets.   They make all of their observations from the Earth that moves so fast in its orbit around the Sun that they must include the theory of relativity in their calculations. Exoplanets & Planet Hunters.
    USA_060516_091_rwx.jpg
  • Physics: NASA/AMES Researchers in Mountain View, California. D. Hudgins, J Dworkin, M. Berstein (Left to Right). Looking for P.A.H. in the lab at Nasa Ames. Polycyclic Aromatic Hydrocarbons (PAHs) are a class of very stable organic molecules made up of only carbon and hydrogen. Photographed at NASA's Ames Research Center, California, USA.- Origin of Life 1999.
    USA_SCI_PHY_23_xs.jpg
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Peter Menzel Photography

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