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PATRICK CHAMPEY, (LEFT), DICK GATES, (RIGHT), AND BILL PODGORSKI, (SEATED), ALIGN SUN SENSOR TO HI-C TELESCOPE USING THEODOLITE
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NASA Administrator Jared Isaacman participates in a formation flight with his F-5 aircraft during an air show performance at the SUN ’n FUN Aerospace Expo, Wednesday, Apr. 15, 2026, in Lakeland, Fla. Isaacman was joined by pilots Sean Gustafson, senior adviso…
Ver en NASA ↗NASA Administrator Jared Isaacman participates in a formation flight with his F-5 aircraft during an air show performance at the SUN ’n FUN Aerospace Expo, Wednesday, Apr. 15, 2026, in Lakeland, Fla. Isaacman was joined by pilots Sean Gustafson, senior adviso…
Ver en NASA ↗NASA Administrator Jared Isaacman participates in a formation flight with his F-5 aircraft during an air show performance at the SUN ’n FUN Aerospace Expo, Wednesday, Apr. 15, 2026, in Lakeland, Fla. Isaacman was joined by pilots Sean Gustafson, senior adviso…
Ver en NASA ↗NASA Administrator Jared Isaacman participates in a formation flight with his F-5 aircraft during an air show performance at the SUN ’n FUN Aerospace Expo, Wednesday, Apr. 15, 2026, in Lakeland, Fla. Isaacman was joined by pilots Sean Gustafson, senior adviso…
Ver en NASA ↗NASA Administrator Jared Isaacman participates in a formation flight with his F-5 aircraft during an air show performance at the SUN ’n FUN Aerospace Expo, Wednesday, Apr. 15, 2026, in Lakeland, Fla. Isaacman was joined by pilots Sean Gustafson, senior adviso…
Ver en NASA ↗NASA's Solar Dynamics Observatory shows a minor eruption of charged particles rising up and twisting about before falling back into the Sun in this close-up of the Sun from a two-hour period on Aug. 13, 2018.
Ver en NASA ↗This diagram illustrates the locations of the star systems closest to the sun. The year when the distance to each system was determined is listed after the system name.
Ver en NASA ↗The artist concept on left is based on theoretical models predicting the direction and strength of magnetic field lines coming from the sun and interstellar space.
Ver en NASA ↗A solar magnetic active region containing the largest sunspot group of the last 10 years unleashed a large (X1.2) flare when it was facing right towards Earth. The flare was associated with a bright coronal mass ejection that emerges from the lower right (Ja…
Ver en NASA ↗The sun emitted a significant solar flare, peaking at 12:22 p.m. EDT on March 11, 2015. NASA’s Solar Dynamics Observatory, which watches the sun constantly, captured an image of the event. Solar flares are powerful bursts of radiation. Harmful radiation from …
Ver en NASA ↗On Nov. 22, 2014 from 5:29 to 6:04 p.m. EST., the moon partially obscured the view of the sun from NASA's Solar Dynamics Observatory. This phenomenon, which is called a lunar transit, could only be seen from SDO's point of view. In 2014, SDO captured four su…
Ver en NASA ↗A coronal mass ejection, or CME, surged off the side of the sun on May 9, 2014, and NASA's newest solar observatory caught it in extraordinary detail. This was the first CME observed by the Interface Region Imaging Spectrograph, or IRIS, which launched in Jun…
Ver en NASA ↗At any given moment, as many as 10 million wild jets of solar material burst from the sun’s surface. They erupt as fast as 60 miles per second, and can reach lengths of 6,000 miles before collapsing. These are spicules, and despite their grass-like abundance,…
Ver en NASA ↗NASA's Solar Dynamics Observatory observed a small prominence, slowly rising further up above the sun, then fell apart and back into the sun over about seven hours (Dec. 6, 2017).
Ver en NASA ↗On Sept. 13, 2015, as NASA Solar Dynamics Observatory, or SDO, kept up its constant watch on the sun. Just as the moon came into SDO field of view on a path to cross the sun, Earth entered the picture, blocking SDO view completely.
Ver en NASA ↗A dark, elongated filament rose up and broke to the lower left and out from the sun seen by NASA's Solar Dynamics Observatory, Apr.9-10, 2017. Filaments are cooler clouds of plasma tethered above the sun surface by magnetic forces.
Ver en NASA ↗On August 31, 2012 a long filament of solar material that had been hovering in the sun's atmosphere, the corona, erupted out into space at 4:36 p.m. EDT. The coronal mass ejection, or CME, traveled at over 900 miles per second. The CME did not travel directly…
Ver en NASA ↗NASA release July 27, 2011 These jets, known as spicules, were captured in an SDO image on April 25, 2010. Combined with the energy from ripples in the magnetic field, they may contain enough energy to power the solar wind that streams from the sun toward Ea…
Ver en NASA ↗This artist concept shows NASA Voyager 1 spacecraft in a new region at the edge of our solar system where the magnetic field lines generated by our sun are piling up and intensifying.
Ver en NASA ↗This artist concept shows NASA Voyager 1 spacecraft exploring a region called the depletion region or magnetic highway at the outer limits of our heliosphere, the bubble the sun blows around itself.
Ver en NASA ↗This artist concept shows NASA two Voyager spacecraft exploring a turbulent region of space known as the heliosheath, the outer shell of the bubble of charged particles around our sun.
Ver en NASA ↗NASA Extreme Ultraviolet Imaging Telescope aboard ESA’s SOHO spacecraft took this image of a huge, handle-shaped prominence in 1999. Prominences are huge clouds of relatively cool dense plasma suspended in the Sun hot, thin corona.
Ver en NASA ↗This artist concept shows the different expected directions of the magnetic fields in interstellar space black lines and the magnetic field emanating from our sun white lines as NASA Voyager 1 spacecraft travels northward out of the heliosphere.
Ver en NASA ↗Contenido y metadatos proporcionados por la NASA Image and Video Library.