81 résultats pour "solar"

• Solar System - astronomy.

  dwarf planets according to the IAU because they have rounded shapes from their own gravity but have not cleared their neighborhoods in space of other objects—bothorbit through the Kuiper Belt, a region beyond Neptune containing thousands of small icy bodies. Pluto and Eris are composed of layers of ice around a rocky core.Ceres qualifies as a dwarf planet because it is spherical but is found in the asteroid belt, a zone between the orbits of Mars and Jupiter that contains thousands of smallrocky...

• Sistema Solar - ciencia y tecnologia.

  pequeños y se componen sobre todo de roca y hierro. Los exteriores son mayores y se componen, principalmente, de hidrógeno, hielo y helio. El Sistema Solar© Microsoft Corporation. Reservados todos los derechos. Mercurio es muy denso, en apariencia debido a su gran núcleo compuesto de hierro. Con una atmósfera tenue, Mercurio tiene una superficie marcada por impactos deasteroides. Venus tiene una atmósfera de dióxido de carbono (CO 2) 90 veces más densa que la de la Tierra; esto causa un efecto i...

• SOLARIS

• El Sistema Solar - (exposé gratuit en espagnol).

• EL SOLAR DE DON RAMIRO

  3 -:.· Cudles fueron aquellos tiempos en qite -'e defendiô ra puerta a fiechazos? r:· Qué recuerda el "cinre/adc' aldal!ôn de alfiÛ;i alcdzar andaluz » ? 4 r:· J\lo hay entre el solar v el hidalgo cierlas corrt.'f111ndencias EJERCIC!O GRAMATICAL J'achèterai un cheval qu(' je puisse à la fois 1nontcr et atteler. Vous n'avez qu'à tlire, et je vous instruirai de tout ce que vous souhaiterez. Quand tu auras un peu plus vécu, la vie t...

• Sol - ciencia y tecnologia.

  3 COMPOSICIÓN Y ESTRUCTURA Interior del SolEntre las regiones del Sol están el núcleo, la zona de radiación, la zona de convección y la fotosfera. Los gases del núcleo son unas150 veces más densos que el agua y alcanzan temperaturas de 16 millones de grados centígrados. La energía del Sol se produce enel núcleo mediante la fusión de los núcleos de hidrógeno en núcleos de helio. En la zona de radiación, la radiación electromagnéticafluye hacia el exterior en forma de calor, y los gases son tan d...

• Eclipse - astronomy.

  bending of light rays passing close to the sun because of the sun’s gravitational field ( see Relativity). The great brilliance of the solar disk and the sun-induced brightening of the earth’s atmosphere make observations of the corona and nearby stars impossible except during a solar eclipse. The coronagraph, a photographictelescope, permits direct observation of the edge of the solar disk at all times. Today, scientific solar eclipse observations are extremely valuable, particularly when thepa...

• Comet - astronomy.

  may exceed the planet Jupiter in size, however. Observations from telescopes on Earth and in space indicate that most of the gases in the coma and tail of a comet are fragmentary molecules, or radicals, of the mostcommon elements in space: hydrogen, carbon, nitrogen, and oxygen. The radicals, for example, of CH, NH, and OH may be broken away from the stable molecules CH 4 (methane), NH 3 (ammonia), and H 2O (water), which may exist as ices or more complex, very cold compounds in the nucleus. Al...

• Kuiper Belt - astronomy.

  III RESEARCH The Kuiper Belt is an exciting area of research in astronomy. The discovery and astronomical exploration of the Kuiper Belt over the past decade have fueled arevolution in scientists’ views of the solar system. Today astronomers recognize the Kuiper Belt as the third major region of the solar system (the other two regions arethe inner solar system, with its small rocky planets, and the outer solar system, with its gas-giant planets). They believe that the belt helps explain Pluto’...

• Planetary Science - astronomy.

  III ORIGINS AND COMPOSITIONS OF PLANETS Astronomers believe that planetary systems are formed of elemental materials that were created in the interiors of giant stars. Some of this material comes from giantstars that shed material into space as they age. Most of the matter to form planets, however, comes from stars that explode as supernovas and spread debris enrichedwith the heavier chemical elements into space. According to the currently accepted views, the most likely first stage in the evo...

• Artificial Satellite - astronomy.

  The first stage of a multistage rocket consists of rocket engines that provide a huge amount of force, or thrust. The first stage lifts the entire launch vehicle—with itsload of fuel, the rocket body, and the satellite—off the launch pad and into the first part of the flight. After its engines use all their fuel, the first stage portion of therocket separates from the rest of the launch vehicle and falls to Earth. The second stage then ignites, providing the energy necessary to lift the satellit...

• Asteroid - astronomy.

  Asteroids of the S type, related to the stony iron meteorites, make up about 15 percent of the total population of asteroids that can be seen from Earth. Much rarer arethe M-type objects, corresponding in composition to the meteorites known as “irons.” These objects are made up of an iron-nickel alloy and may represent the cores ofbodies that were large enough to differentiate into layers and to melt deep inside. Their rocky outer layers may have been removed by impacts with other asteroids . A...

• Jupiter (planet) - astronomy.

  Beneath the supercritical fluid zone, the pressure reaches 3 million Earth atmospheres. At this depth, the atoms collide so frequently and violently that the hydrogenatoms are ionized—that is, the negatively charged electrons are stripped away from the positively charged protons of the hydrogen nuclei. This ionization results in asea of electrically charged particles that resembles a liquid metal and gives rise to Jupiter’s magnetic field. This liquid metallic hydrogen zone is 30,000 to 40,000 k...

• Extrasolar Planets - astronomy.

  When a planet passes in a front of the star it orbits—an event called a transit—it causes a small dip in the brightness of the star. Measuring the slight change in thebrightness can be used not only to directly detect a planet, but to determine its size and orbit. However, the planet needs to orbit in a plane that lies in a telescope’sline of sight on the star. Despite long odds, Earth-based telescopes have detected and studied a few exoplanets using this method. The first space telescope design...

• Clima - ciencias de la naturaleza.

  2 CLIMATOLOGÍA Y ATMÓSFERA La climatología es una ciencia diferente a la meteorología, aunque se basa en sus análisis. La meteorología es la ciencia que estudia los fenómenos atmosféricos (viento,lluvia, aurora boreal, rayo...) y los mecanismos que producen el tiempo atmosférico actual; una de sus finalidades es elaborar pronósticos sobre el tiempo que hará en elfuturo. La climatología estudia la regularidad del tiempo, y se diferencia de la meteorología en que trabaja con datos medios en vez d...

• Venus (planet) - astronomy.

  level winds circle the planet at 360 km/h (225 mph), making a complete rotation in only four days. These winds are said to super-rotate because they travel muchfaster than the rotation of the planet itself. These high-speed winds cover the planet completely, blowing toward the west at virtually every latitude from equator topole. The motions of descending probes, however, have shown that the bulk of Venus’s tremendously dense atmosphere, closer to the planet’s surface, is almoststagnant. From th...

• Neptune (planet) - astronomy.

  The gaseous atmosphere of Neptune contains hydrogen, helium, and about 3 percent methane. It extends about 5,000 km (about 3,000 mi) above the planet’s ocean.Light reflected from Neptune’s deep atmosphere is blue, because the atmospheric methane absorbs red and orange light but scatters blue light. In 1998 astronomersalso identified molecules of methyl in Neptune’s atmosphere. Methyl molecules each contain one carbon atom and three hydrogen atoms. Methyl molecules are knownas hydrocarbon radical...

• Clima - geografía.

  2 CLIMATOLOGÍA Y ATMÓSFERA La climatología es una ciencia diferente a la meteorología, aunque se basa en sus análisis. La meteorología es la ciencia que estudia los fenómenos atmosféricos (viento,lluvia, aurora boreal, rayo...) y los mecanismos que producen el tiempo atmosférico actual; una de sus finalidades es elaborar pronósticos sobre el tiempo que hará en elfuturo. La climatología estudia la regularidad del tiempo, y se diferencia de la meteorología en que trabaja con datos medios en vez d...

• Clima - geografía.

  2 CLIMATOLOGÍA Y ATMÓSFERA La climatología es una ciencia diferente a la meteorología, aunque se basa en sus análisis. La meteorología es la ciencia que estudia los fenómenos atmosféricos (viento,lluvia, aurora boreal, rayo...) y los mecanismos que producen el tiempo atmosférico actual; una de sus finalidades es elaborar pronósticos sobre el tiempo que hará en elfuturo. La climatología estudia la regularidad del tiempo, y se diferencia de la meteorología en que trabaja con datos medios en vez d...

• Clima - ciencias de la naturaleza.

  2 CLIMATOLOGÍA Y ATMÓSFERA La climatología es una ciencia diferente a la meteorología, aunque se basa en sus análisis. La meteorología es la ciencia que estudia los fenómenos atmosféricos (viento,lluvia, aurora boreal, rayo...) y los mecanismos que producen el tiempo atmosférico actual; una de sus finalidades es elaborar pronósticos sobre el tiempo que hará en elfuturo. La climatología estudia la regularidad del tiempo, y se diferencia de la meteorología en que trabaja con datos medios en vez d...

• Sun - astronomy.

  A The Sun’s Place in the Milky Way The Milky Way Galaxy contains about 400 billion stars. All of these stars, and the gas and dust between them, are rotating about a galactic center. Stars that arefarther away from the center move at slower speeds and take longer to go around it. The Sun is located in the outer part of the galaxy, at a distance of 2.6 × 10 17 km (1.6 × 10 17 mi) from the center. The Sun, which is moving around the center at a velocity of 220 km/s (140 mi/s), takes 250 million y...

• Supernova - astronomy.

  The term hypernova has been proposed for an extremely massive core-collapse supernova—possibly more than 100 times the mass of the Sun. A hypernova is thought to form a black hole. Just before it explodes, a hypernova may release a huge burst of gamma rays in a jet from the rotating black hole at its center. These jets mayexplain the so-called long gamma-ray bursts detected by astronomers. According to some researchers, massive stars with over 40 solar masses may sometimescollapse directly int...

• Radio Astronomy - astronomy.

  equivalent to the apparent angular dimensions of a basketball at the distance of the moon. In 1984, the U.S. government appropriated funds for the construction of aninstallation called the very long baseline array (VLBA), a network of 10 radio antennas spread from the U.S.-Canadian border to Puerto Rico and from Hawaii to the U.S.Atlantic coast. The VLBA is expected to provide angular resolutions in the range of 200-millionths of an arc second. Canada and Australia are both planning similarprogr...

• Voyager - astronomy.

  Voyager 1 had not yet reached the termination shock boundary. They reported that the spacecraft was near but not yet there. Both teams agreed, nevertheless, thatVoyager 1 had entered unknown territory and had embarked on the final phase of its mission, which includes exploring the termination shock boundary, the heliopauseitself, and finally, interstellar space. Voyager 2 is also due to explore these outer regions. Unlike Voyager 1, a key instrument known as a plasma detector is still functionin...

• Mercury (planet) - astronomy.

  In 1991 powerful radio telescopes on Earth revealed signs of possible deposits of ice in the polar regions of Mercury. These ice deposits occur in areas where sunlightnever falls, such as crater bottoms near both of the planet’s poles. Similar ice deposits may have been found during the 1990s near the poles of the Moon by theClementine and Lunar Prospector spacecrafts. The ice on Mercury likely comes from comets or water-bearing meteorites that have hit Mercury over the planet’s historyup throug...

• Natural Satellite - astronomy.

  Titan, Saturn’s largest moon, also has few impact craters. Although icy volcanism from water and ammonia may occur along with some tectonic activity, Titan’s youngsurface is most likely the result of weather processes. Titan’s dense, cold atmosphere precipitates particles of complex organic molecules that accumulate as dunes andmountains. Methane rain erodes the surface and creates lakes at the moon’s poles. Triton’s young surface also may result from processes in its atmosphere, as well aserupt...

• Astrobiology - astronomy.

  water to help reactions along. American chemists Stanley Miller and Harold Urey tested part of Oparin and Haldane’s hypothesis in the early 1950s by simulating conditions of the early Earth. In whathas become known as the Miller-Urey experiment, the two scientists connected two flasks with a loop of glass tubing that allowed the gases to pass between the flasks.They filled the upper flask with methane, ammonia, and hydrogen—components thought to have been in the early atmosphere. They filled the...

• La exploración del espacio - (exposé gratuit en espagnol).

  dos horas por nuestro satélite. Recogieron 21 kg de muestras del suelo, tomaron fotografías y colocaron un artefacto para detectar ymedir el viento solar, un reflector de rayos láser y un sismógrafo. Comprobaron que no era difícil caminar y correr bajo una gravedadseis veces menor que la de la Tierra. Millones de personas pudieron seguir en directo la retransmisión vía satélite del acontecimiento. El regreso del Apolo 11 se realizó sin contratiempos y la nave cayó en aguas del océano Pacífico,...

• History of Astronomy - astronomy.

  Egypt, the Sun was directly overhead at noon. On the same date and time in Alexandria, Egypt, the Sun was about 7 degrees south of zenith. With simple geometryand knowledge of the distance between the two cities, he estimated the circumference of the Earth to be 250,000 stadia. (The stadium was a unit of length, derivedfrom the length of the racetrack in an ancient Greek stadium. We have an approximate idea of how big an ancient Greek stadium was, and based on that approximationEratosthenes was...

• Star (astronomy) - astronomy.

  absorbing the missing colors of light. For example, the set of dark lines made by hydrogen includes a dark red line, the set of dark lines made by sodium includes a pairof dark yellow lines, and the set of dark lines made by iron includes lines of nearly every color. Each element in the gaseous outer layer of a star produces its ownparticular pattern of dark spectrum lines, depending on the temperature and pressure of the gas. Astronomers have observed spectrum lines, or spectra, for hundredsof...

• Mars (planet) - astronomy.

  The Martian core is probably much like Earth’s, consisting mostly of iron, with a small amount of nickel. If other light elements, particularly sulfur, exist there as well, thecore may be larger than presently thought. From studying Earth’s magnetic field and core, scientists theorize that the motions of the liquid rock in Earth’s core generateits magnetic field. Mars does not have a significant magnetic field, so scientists believe that Mars’s core is probably solid. However, spacecraft data in...

• Orientación espacial 1 INTRODUCCIÓN Orientación espacial, posición de un punto, lugar, objeto o persona sobre la superficie terrestre respecto a un sistema de referencia.

  En los últimos años han aparecido instrumentos y técnicas muy precisos para determinar la posición de un punto de la Tierra: informan sobre su latitud, su longitud e,incluso, su altitud. Son las redes de localización por satélite, y muchas personas las utilizan en lugar de las brújulas. El más conocido es el Sistema de Posicionamiento Global (GPS), Global Positioning System en inglés, que surgió para que las naves militares estadounidenses realizaran trayectos más seguros. Aunque en origen era...

• Saturn - astronomy.

  measurements of the magnetic field made by the Voyager space probes in the 1980s. Additional Cassini findings reported in March 2007 suggested that particles originating from geysers on the moon Enceladus may provide a partial explanation for thechange. The neutral gas particles become electrically charged and are captured by Saturn’s magnetic field, forming a disk of hot, ionized gas around the planet’sequator. The charged particles interact with the magnetic field and slow down the rotation of...

• Eclipse - ciencia y tecnologia.

  Eclipse anularUn eclipse anular se produce cuando la Luna está cerca de su apogeo (el punto de su órbita en el que se encuentra más distante de laTierra), al interponerse entre el Sol y la Tierra. En estos eclipses permanece visible un anillo del disco solar. Esta imagen fue tomadaen Kenia durante un eclipse que tuvo lugar el 16 de febrero de 1980.M.P. Kahl/Photo Researchers, Inc. En áreas fuera de la banda barrida por la sombra de la Luna, pero dentro de la penumbra, tienen lugar eclipses parci...

• Pioneer (spacecraft) - astronomy.

  The Pioneer Venus spacecraft contributed a tremendous amount of new information about Venus. Venus showed an enormous difference between night (-170°C, or -274°F) and day (40°C, or 104°F) temperatures in the highest regions of the atmosphere (the thermosphere during the day and the cryosphere at night) at altitudesbetween 130 and 200 km (between 81 and 120 mi). Below the clouds was a region of constantly high temperature and pressure and almost no wind. The Pioneer Venuscraft found the clouds ar...

• Desarrollo de los sistemas planetarios - ciencia y tecnologia.

  Incluso después de que los cuatro cuerpos principales que se convertirían en los planetas interiores hubieran tomado forma en el disco de material situado en torno al jovenSol, existían muchos pedazos de escombros más pequeños en el Sistema Solar interior, que seguían sus propias órbitas y eran absorbidos por los cuatro planetas al pasarcerca de ellos. Los cráteres de la superficie lunar muestran el efecto del bombardeo que continuó después de la formación de los planetas; las sondas espaciales...

• World Energy Supply.

  In the 1990s, oil production by non-OPEC countries remained strong and production by OPEC countries rebounded. The result at the end of the 20th century was aworld oil surplus and prices (when adjusted for inflation) that were lower than in 1972. Experts are uncertain about future oil supplies and prices. Low prices have spurred greater oil consumption, and experts question how long world petroleum reservescan keep pace with increased demand. Many of the world’s leading petroleum geologists beli...

• Pluto - astronomy.

  depended on how Pluto was classified. The status of Pluto drew world attention in 2006 when the official body that governs the naming of astronomical objects, the International Astronomical Union (IAU),voted for an official definition of the term planet . According to the standards adopted, a “classical planet” must orbit the Sun, must have a rounded shape from effects of its own gravity, and must be the dominant object in its region of space, having cleared the neighborhood of its orbit of oth...

• Moon - astronomy.

  B Volcanic Features Maria, domes, rilles, and a few craters display indisputable characteristics of volcanic origin. Maria are plains of dark-colored rock that cover approximately 40 percent ofthe Moon's visible hemisphere. The maria formed when molten rock erupted onto the surface and solidified between 3.16 billion and 3.96 billion years ago. This rockresembles terrestrial basalt, a volcanic rock type widely distributed on Earth, but the rock that formed the maria has a higher iron content an...

• Ecología - ciencias de la naturaleza.

  PraderaLas praderas forman una zona ecológica que se extiende entre los desiertos y los bosques templados, e incluyen gran variedad decomunidades vegetales. Propias, por lo general, del interior de los continentes, las praderas se componen de hierbas, vegetaciónherbácea perenne y gramíneas. Se cultivan y explotan como pastos. Si se sobreexplotan, el suelo puede quedar denudado y expuestoa la erosión, proceso llamado desertización.John Bova/Photo Researchers, Inc. Bajo la influencia de la latitud...

• Native American Architecture I INTRODUCTION Native American Architecture, traditional architecture of the peoples of who lived in North America before Europeans arrived.

  Mound Builders who resided in the area.John Elk III/Bruce Coleman, Inc. Another mound building culture, named Hopewell, also appears to have originated in Ohio but expanded west to Iowa, Kansas, and Oklahoma, south to Louisiana,Mississippi, and Alabama, east to Georgia and the Appalachian Mountains, and north to Wisconsin, Michigan, and lower Ontario in Canada. The Hopewell culture lastedfrom about 200 BC to 400 AD. Hopewell people built large, linear mounds to create enclosures in geometrical...

• Cambio climático - ciencias de la naturaleza.

  relevante que influye en la dinámica del clima en la Tierra. El hielo presente en las regiones polares proporciona datos sobre la composición de la antigua atmósfera de la Tierra. Los núcleos de hielo analizados por los científicos,procedentes de las placas de hielo de Groenlandia y de la Antártida, ofrecen información sobre la temperatura y los gases de efecto invernadero presentes en la atmósferade hace cientos de miles de años. Las capas de estos núcleos de hielo formadas por las nevadas esta...

• Light - astronomy.

  Each different frequency or wavelength of visible light causes our eye to see a slightly different color. The longest wavelength we can see is deep red at about 700 nm.The shortest wavelength humans can detect is deep blue or violet at about 400 nm. Most light sources do not radiate monochromatic light. What we call white light,such as light from the Sun, is a mixture of all the colors in the visible spectrum, with some represented more strongly than others. Human eyes respond best to greenlight...

• Saturno (planeta) - ciencia y tecnologia.

  atmósfera de Saturno hace que la presión atmosférica aumente con rapidez hacia el interior, donde el hidrógeno se hace líquido. Hacia el centro del planeta el hidrógenolíquido se condensa en hidrógeno metálico, que es un conductor eléctrico. Las corrientes eléctricas presentes en este hidrógeno metálico son las responsables del campomagnético del planeta. En el centro de Saturno se han consolidado, probablemente, elementos pesados formando un pequeño núcleo rocoso a una temperatura cercana alos...

• Radioastronomía - ciencia y tecnologia.

  305 m de diámetro. Las mayores antenas parabólicas dirigibles de plato miden de 50 a 100 m de diámetro y tienen una resolución de 1 minuto de arco aproximadamente,equivalente a la del ojo humano en longitudes de onda ópticas. Las ondas de radio que entran son enfocadas por la superficie parabólica en una pequeña antena de cuernosque las conduce a un receptor de radio extremadamente sensible. Estos receptores, aunque similares en principio a los aparatos de radio domésticos, detectan señales tand...

• Infrared Space Observatory - astronomy.

  know how often these disks occur around stars to help them understand how common it is for planets to form. ISO found several previously unknown stars with disks.ISO also detected olivine, a silicate mineral found in Earth’s own rocky mantle, in the comet Hale-Bopp, which was visible from Earth in 1996 and 1997. The discovery ofolivine in the comet suggests that the comet and Earth have a similar origin. The satellite also detected the first evidence of water outside of the solar system inplanet...

• expose londre

  L'intensité de l'énergie solaire varie en permanence L'excédent d'énergie doit donc être stocké pour répondre aux besoins en cas de manque de soleil dans des batteries. Le 26 avril a lieu le premier essai roulant de SOLARIS 1 dans l’enceinte du lycée. Le véhicule traverse l’établissement, faisant la preuve d’une stabilité et d’une maniabilité encourageantes. Du mercredi 28 JUIN au Dimanche 2 Juillet le projet est expo...

• Uranus (planet) - astronomy.

  V COMPOSITION AND STRUCTURE A Interior of Uranus Uranus contains mostly rock and water, with hydrogen and helium (and trace amounts of methane) in its dense atmosphere. Astronomers believe that Uranus, likeNeptune, formed from the same material—principally frozen water and rock—that composes most of the planet’s moons. As the planet grew, pressures andtemperatures in the planet’s interior increased, heating the planet’s frozen water into a hot liquid. Uranus probably has a relatively small roc...

• Bacteria - ciencias de la naturaleza.

  2.3 Bacterias autótrofas y heterótrofas Respecto a la fuente de carbono que utilizan para nutrirse, las bacterias se pueden clasificar en autótrofas y heterótrofas. Las bacterias autótrofas (producen su propioalimento), lo obtienen del dióxido de carbono (CO 2). Sin embargo, la mayoría de las bacterias son heterótrofas (no producen su propio alimento) y obtienen el carbono de nutrientes orgánicos como el azúcar. Algunas especies heterótrofas sobreviven como parásitos, creciendo dentro de otros...

• Vía Láctea - ciencia y tecnologia.

  población I, junto con mucho polvo interestelar y gas. Un brazo pasa por las proximidades del Sol e incluye a la gran nebulosa de Orión. 4 ROTACIÓN La Vía Láctea gira alrededor de un eje que une los polos galácticos. Contemplada desde el polo norte galáctico, la rotación de la Vía Láctea se produce en el sentido de lasagujas del reloj, arrastrando los brazos espirales. El periodo de rotación aumenta cuando disminuye la distancia desde el centro del sistema galáctico. En las proximidadesdel Sist...