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astronomy
astronomy

... List and explain the kinds of information that can be obtained by analyzing the spectra of astronomical objects. Chapter 16 Summarize the overall properties of the Sun. Explain how energy travels from the solar core, through the interior, and out into space. Name the Sun’s outer layers and describe ...
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... As the Local Interstellar Wind blows through our solar system, it must pass through another wind—that produced by our own sun. The solar wind is a hot plasma—consisting of charged particles (mostly protons, helium nuclei and electrons)—that streams outward from the sun at high speed. Its source is t ...
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... therefore supposed to be @ E 3.50 / N44.52 . The report reads: "Eleven hundred after seventy eight, the Moon hid the Sun in its 21st day". Only the year is mentioned, what is already most precious, but "its 21st day" is a weird way of describing the new Moon. ...
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... developed a calibration facility to accurately measure particles in the submicrometer size range. The measurement facility is now offered as a special test, but it will become a NIST calibration service as demand for these measurements increases. The NIST calibration facility uses electrical differe ...
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... which are thrown out by volcanoes at eruption. Rising on the top of atmosphere the particles with critical masses can circulate there a long time. The part of them accumulates on the surface; another part comes into cosmic space. A source of aerosols is also the large meteorites. At collision of a m ...
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... The primary goal of the Helioseismic and Magnetic Imager (HMI) investigation is to study the origin of solar variability and to characterize and understand the Sun’s interior and the various components of magnetic activity. The HMI investigation is based on measurements obtained with the HMI instrum ...
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... were revealed by the ROSAT all-sky survey. The XMM-Newton observatory allows us to resolve more point sources than ever before. When these are removed, spectra of the underlying soft x-ray background (SXRB) can be extracted and high resolution spectroscopy performed. ...
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... Cosmochemistry [19], and debated there [18-21] and in Science [22,23]. Advocates of in situ super-heavy element fission as the source of excess 136Xe in meteorites published a supporting study in the Proceedings of the National Academy of Science [24]. Another group proposed that excess 136Xe might ...
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Advanced Composition Explorer



Advanced Composition Explorer (ACE) is a NASA Explorers program Solar and space exploration mission to study matter comprising energetic particles from the solar wind, the interplanetary medium, and other sources. Real-time data from ACE is used by the NOAA Space Weather Prediction Center to improve forecasts and warnings of solar storms. The ACE robotic spacecraft was launched August 25, 1997 and entered a Lissajous orbit close to the L1 Lagrangian point (which lies between the Sun and the Earth at a distance of some 1.5 million km from the latter) on December 12, 1997. The spacecraft is currently operating at that orbit. Because ACE is in a non-Keplerian orbit, and has regular station-keeping maneuvers, the orbital parameters at right are only approximate. The spacecraft is still in generally good condition in 2015, and is projected to have enough fuel to maintain its orbit until 2024. NASA Goddard Space Flight Center managed the development and integration of the ACE spacecraft.
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