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Vega Deutschland

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Thus, for many years, Vega was used as a baseline for the calibration of absolute photometric brightness scales. This approach is more convenient for astronomers, since Vega is not always available for calibration and varies in brightness.

The UBV photometric system measures the magnitude of stars through ultraviolet , blue, and yellow filters, producing U , B , and V values, respectively.

Vega is one of six A0V stars that were used to set the initial mean values for this photometric system when it was introduced in the s.

In effect, the magnitude scale has been calibrated so that the magnitude of these stars is the same in the yellow, blue, and ultraviolet parts of the electromagnetic spectrum.

This range of variability was near the limits of observational capability for that time, and so the subject of Vega's variability has been controversial.

The magnitude of Vega was measured again in at the David Dunlap Observatory and showed some slight variability.

Thus it was suggested that Vega showed occasional low-amplitude pulsations associated with a Delta Scuti variable. Thus the variability was thought to possibly be the result of systematic errors in measurement.

Vega became the first solitary main-sequence star beyond the Sun known to be an X-ray emitter when in it was observed from an imaging X-ray telescope launched on an Aerobee from the White Sands Missile Range.

The Infrared Astronomical Satellite IRAS discovered an excess of infrared radiation coming from the star, and this was attributed to energy emitted by the orbiting dust as it was heated by the star.

Vega's spectral class is A0V, making it a blue-tinged white main sequence star that is fusing hydrogen to helium in its core. Since more massive stars use their fusion fuel more quickly than smaller ones, Vega's main-sequence lifetime is roughly one billion years, a tenth of the Sun's.

After leaving the main sequence, Vega will become a class-M red giant and shed much of its mass, finally becoming a white dwarf. At present, Vega has more than twice the mass [21] of the Sun and its bolometric luminosity is about 40 times the Sun's.

Because it is rapidly-rotating and seen nearly pole-on, its apparent luminosity, calculated assuming it was the same brightness all over, is about 57 times the Sun's.

Most of the energy produced at Vega's core is generated by the carbon—nitrogen—oxygen cycle CNO cycle , a nuclear fusion process that combines protons to form helium nuclei through intermediary nuclei of carbon, nitrogen, and oxygen.

The CNO cycle is highly temperature sensitive, which results in a convection zone about the core [57] that evenly distributes the 'ash' from the fusion reaction within the core region.

The overlying atmosphere is in radiative equilibrium. This is in contrast to the Sun, which has a radiation zone centered on the core with an overlying convection zone.

The energy flux from Vega has been precisely measured against standard light sources. Using spectropolarimetry , a magnetic field has been detected on the surface of Vega by a team of astronomers at the Observatoire du Pic du Midi.

This is the first such detection of a magnetic field on a spectral class A star that is not an Ap chemically peculiar star.

Vega has a rotation period of When the radius of Vega was measured to high accuracy with an interferometer , it resulted in an unexpectedly large estimated value of 2.

However, this discrepancy can be explained if Vega is a rapidly rotating star that is being viewed from the direction of its pole of rotation.

The pole of Vega—its axis of rotation—is inclined no more than five degrees from the line-of-sight to the Earth.

At the high end of estimates for the rotation velocity for Vega is The estimated polar radius of this star is 2.

As viewed from the poles, this results in a darker lower-intensity limb than would normally be expected for a spherically symmetric star.

The temperature gradient may also mean that Vega has a convection zone around the equator, [12] [70] while the remainder of the atmosphere is likely to be in almost pure radiative equilibrium.

As a result, if Vega were viewed along the plane of its equator instead of almost pole-on, then its overall brightness would be lower.

As Vega had long been used as a standard star for calibrating telescopes, the discovery that it is rapidly rotating may challenge some of the underlying assumptions that were based on it being spherically symmetric.

With the viewing angle and rotation rate of Vega now better known, this will allow improved instrument calibrations.

In astronomy, those elements with higher atomic numbers than helium are termed "metals". The unusually low metallicity of Vega makes it a weak Lambda Boötis star.

One possibility is that the chemical peculiarity may be the result of diffusion or mass loss, although stellar models show that this would normally only occur near the end of a star's hydrogen-burning lifespan.

Another possibility is that the star formed from an interstellar medium of gas and dust that was unusually metal-poor.

The observed helium to hydrogen ratio in Vega is 0. This may be caused by the disappearance of a helium convection zone near the surface.

Energy transfer is instead performed by the radiative process , which may be causing an abundance anomaly through diffusion.

The radial velocity of Vega is the component of this star's motion along the line-of-sight to the Earth. Movement away from the Earth will cause the light from Vega to shift to a lower frequency toward the red , or to a higher frequency toward the blue if the motion is toward the Earth.

Thus the velocity can be measured from the amount of shift of the star's spectrum. Motion transverse to the line of sight causes the position of Vega to shift with respect to the more distant background stars.

Careful measurement of the star's position allows this angular movement, known as proper motion , to be calculated. Vega's proper motion is The net proper motion of Vega is Although Vega is at present only the fifth-brightest star in the night sky, the star is slowly brightening as proper motion causes it to approach the Sun.

Based on this star's kinematic properties, it appears to belong to a stellar association called the Castor Moving Group.

However, Vega may be much older than this group, so the membership remains uncertain. All members of the group are moving in nearly the same direction with similar space velocities.

Membership in a moving group implies a common origin for these stars in an open cluster that has since become gravitationally unbound.

One of the early results from the Infrared Astronomy Satellite IRAS was the discovery of excess infrared flux coming from Vega, beyond what would be expected from the star alone.

It was proposed that this radiation came from a field of orbiting particles with a dimension on the order of a millimeter, as anything smaller would eventually be removed from the system by radiation pressure or drawn into the star by means of Poynting—Robertson drag.

This effect is most pronounced for tiny particles that are closer to the star. To maintain this amount of dust in orbit around Vega, a continual source of replenishment would be required.

A proposed mechanism for maintaining the dust was a disk of coalesced bodies that were in the process of collapsing to form a planet.

Following the discovery of an infrared excess around Vega, other stars have been found that display a similar anomaly that is attributable to dust emission.

As of , about of these stars have been found, and they have come to be termed "Vega-like" or "Vega-excess" stars.

It is believed that these may provide clues to the origin of the Solar System. By , the Spitzer Space Telescope had produced high-resolution infrared images of the dust around Vega.

Production of the dust would require collisions between asteroids in a population corresponding to the Kuiper Belt around the Sun. Thus the dust is more likely created by a debris disk around Vega, rather than from a protoplanetary disk as was earlier thought.

The disk of dust is produced as radiation pressure from Vega pushes debris from collisions of larger objects outward. However, continuous production of the amount of dust observed over the course of Vega's lifetime would require an enormous starting mass—estimated as hundreds of times the mass of Jupiter.

Hence it is more likely to have been produced as the result of a relatively recent breakup of a moderate-sized or larger comet or asteroid, which then further fragmented as the result of collisions between the smaller components and other bodies.

This dusty disk would be relatively young on the time scale of the star's age, and it will eventually be removed unless other collision events supply more dust.

Hopkins in , [87] revealed evidence for an inner dust band around Vega. This was hypothesized as either a perturbation of the dust disk by a planet or else an orbiting object that was surrounded by dust.

However, images by the Keck telescope had ruled out a companion down to magnitude 16, which would correspond to a body with more than 12 times the mass of Jupiter.

Determining the nature of the planet has not been straightforward; a paper hypothesizes that the clumps are caused by a roughly Jupiter-mass planet on an eccentric orbit.

Dust would collect in orbits that have mean-motion resonances with this planet—where their orbital periods form integer fractions with the period of the planet—producing the resulting clumpiness.

The migration of this planet would likely require gravitational interaction with a second, higher-mass planet in a smaller orbit. Using a coronagraph on the Subaru telescope in Hawaii in , astronomers were able to further constrain the size of a planet orbiting Vega to no more than 5—10 times the mass of Jupiter.

The observations showed that the debris ring is smooth and symmetric. No evidence was found of the blobs reported earlier, casting doubts on the hypothesized giant planet.

Although a planet has yet to be directly observed around Vega, the presence of a planetary system can not yet be ruled out. Thus there could be smaller, terrestrial planets orbiting closer to the star.

The inclination of planetary orbits around Vega is likely to be closely aligned to the equatorial plane of this star.

From the perspective of an observer on a hypothetical planet around Vega, the Sun would appear as a faint 4.

Among the northern Polynesian people, Vega was known as whetu o te tau , the year star. For a period of history it marked the start of their new year when the ground would be prepared for planting.

Eventually this function became denoted by the Pleiades. In Babylonian astronomy , Vega may have been one of the stars named Dilgan, "the Messenger of Light".

To the ancient Greeks , the constellation Lyra was formed from the harp of Orpheus , with Vega as its handle.

In Zoroastrianism , Vega was sometimes associated with Vanant, a minor divinity whose name means "conqueror". The indigenous Boorong people of northwestern Victoria named it as Neilloan , [] "the flying Loan ".

Further research has been done and this event has been analyzed by Nilesh Oak based upon using astronomical calculations in his book on Mahabharata dating.

Medieval astrologers counted Vega as one of the Behenian stars [] and related it to chrysolite and winter savory. Cornelius Agrippa listed its kabbalistic sign under Vultur cadens , a literal Latin translation of the Arabic name.

Vega became the first star to have a car named after it with the French Facel Vega line of cars from onwards, and later on, in America, Chevrolet launched the Vega in Coordinates : 18 h 36 m From Wikipedia, the free encyclopedia.

This article is about the star. For other uses, see Vega disambiguation. Star in the constellation Lyra. Location of Vega in the constellation Lyra.

Allen's Astrophysical Qualities 4th ed. New York: Springer-Verlag. See: Matteucci, Francesca The Chemical Evolution of the Galaxy.

Astrophysics and Space Science Library. UVW is a Cartesian coordinate system , so the Euclidean distance formula applies.

Oxford English Dictionary 3rd ed. Oxford University Press. September Subscription or UK public library membership required.

Merriam-Webster Dictionary. Cambridge, Massachusetts: Sky Pub. November Astronomy and Astrophysics. The Astronomical Journal.

Bibcode : AJ Originally Published in: yCat Bibcode : yCat Bibcode : yCat. June 20—24, Proceedings from IAU Symposium no. Determination of Radial Velocities and Their Applications.

London, England. Bibcode : IAUS January The Astrophysical Journal. Bibcode : ApJ Astrophysical Journal. Star Names: Their Lore and Meaning. Courier Dover Publications.

Otis Philadelphia: Oxford University Press. Retrieved Susan; et al. JHU Press. Proceedings of the American Philosophical Society.

Bibcode : Natur. Then call us. If you need service, feel free to call our hour hotline, available seven days a week. Only normal call charges are incurred:.

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New VEGABAR compact pressure switches VEGA completes its sensor portfolio and becomes a full-range supplier of pressure measurement technology with sensors for hygiene-sensitive standard applications and demanding measuring tasks.

Radar sensors for the water and wastewater industry VEGA extends its portfolio of level sensors with a radar instrument series for standard measuring tasks and price-sensitive applications.

On an interactive tour, discover typical measuring points for the new compact radar sensors. Level measurement with ultrasonic was yesterday - the future is radar!

Compared to ultrasonic sensors, radar sensors measure unaffected by temperature fluctuations, vacuum or high pressures and are insensitive to contamination.

Discover compact level sensors with 80 GHz radar technology now. Measurement technology for maximum safety in every application VEGA's measurement technology sets new standards in reliability, accuracy and economy for all media and process conditions.

Level and pressure instrumentation for the process industry VEGA is a global manufacturer of sensors for measuring level, point level, pressure as well as devices and software for integrating them into process control systems.

What would you like to measure? Customized measurement technology. Available within a few days. Solutions for a wide variety of industries High vessels, temperatures or pressure.

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Cement Industry. One possibility is that the chemical peculiarity may be the result of diffusion or mass loss, although stellar models show that this would normally only occur near the end of a star's hydrogen-burning lifespan.

Another possibility is that the star formed from an interstellar medium of gas and dust that was unusually metal-poor. The observed helium to hydrogen ratio in Vega is 0.

This may be caused by the disappearance of a helium convection zone near the surface. Energy transfer is instead performed by the radiative process , which may be causing an abundance anomaly through diffusion.

The radial velocity of Vega is the component of this star's motion along the line-of-sight to the Earth. Movement away from the Earth will cause the light from Vega to shift to a lower frequency toward the red , or to a higher frequency toward the blue if the motion is toward the Earth.

Thus the velocity can be measured from the amount of shift of the star's spectrum. Motion transverse to the line of sight causes the position of Vega to shift with respect to the more distant background stars.

Careful measurement of the star's position allows this angular movement, known as proper motion , to be calculated. Vega's proper motion is The net proper motion of Vega is Although Vega is at present only the fifth-brightest star in the night sky, the star is slowly brightening as proper motion causes it to approach the Sun.

Based on this star's kinematic properties, it appears to belong to a stellar association called the Castor Moving Group.

However, Vega may be much older than this group, so the membership remains uncertain. All members of the group are moving in nearly the same direction with similar space velocities.

Membership in a moving group implies a common origin for these stars in an open cluster that has since become gravitationally unbound.

One of the early results from the Infrared Astronomy Satellite IRAS was the discovery of excess infrared flux coming from Vega, beyond what would be expected from the star alone.

It was proposed that this radiation came from a field of orbiting particles with a dimension on the order of a millimeter, as anything smaller would eventually be removed from the system by radiation pressure or drawn into the star by means of Poynting—Robertson drag.

This effect is most pronounced for tiny particles that are closer to the star. To maintain this amount of dust in orbit around Vega, a continual source of replenishment would be required.

A proposed mechanism for maintaining the dust was a disk of coalesced bodies that were in the process of collapsing to form a planet.

Following the discovery of an infrared excess around Vega, other stars have been found that display a similar anomaly that is attributable to dust emission.

As of , about of these stars have been found, and they have come to be termed "Vega-like" or "Vega-excess" stars.

It is believed that these may provide clues to the origin of the Solar System. By , the Spitzer Space Telescope had produced high-resolution infrared images of the dust around Vega.

Production of the dust would require collisions between asteroids in a population corresponding to the Kuiper Belt around the Sun.

Thus the dust is more likely created by a debris disk around Vega, rather than from a protoplanetary disk as was earlier thought.

The disk of dust is produced as radiation pressure from Vega pushes debris from collisions of larger objects outward.

However, continuous production of the amount of dust observed over the course of Vega's lifetime would require an enormous starting mass—estimated as hundreds of times the mass of Jupiter.

Hence it is more likely to have been produced as the result of a relatively recent breakup of a moderate-sized or larger comet or asteroid, which then further fragmented as the result of collisions between the smaller components and other bodies.

This dusty disk would be relatively young on the time scale of the star's age, and it will eventually be removed unless other collision events supply more dust.

Hopkins in , [87] revealed evidence for an inner dust band around Vega. This was hypothesized as either a perturbation of the dust disk by a planet or else an orbiting object that was surrounded by dust.

However, images by the Keck telescope had ruled out a companion down to magnitude 16, which would correspond to a body with more than 12 times the mass of Jupiter.

Determining the nature of the planet has not been straightforward; a paper hypothesizes that the clumps are caused by a roughly Jupiter-mass planet on an eccentric orbit.

Dust would collect in orbits that have mean-motion resonances with this planet—where their orbital periods form integer fractions with the period of the planet—producing the resulting clumpiness.

The migration of this planet would likely require gravitational interaction with a second, higher-mass planet in a smaller orbit.

Using a coronagraph on the Subaru telescope in Hawaii in , astronomers were able to further constrain the size of a planet orbiting Vega to no more than 5—10 times the mass of Jupiter.

The observations showed that the debris ring is smooth and symmetric. No evidence was found of the blobs reported earlier, casting doubts on the hypothesized giant planet.

Although a planet has yet to be directly observed around Vega, the presence of a planetary system can not yet be ruled out. Thus there could be smaller, terrestrial planets orbiting closer to the star.

The inclination of planetary orbits around Vega is likely to be closely aligned to the equatorial plane of this star. From the perspective of an observer on a hypothetical planet around Vega, the Sun would appear as a faint 4.

Among the northern Polynesian people, Vega was known as whetu o te tau , the year star. For a period of history it marked the start of their new year when the ground would be prepared for planting.

Eventually this function became denoted by the Pleiades. In Babylonian astronomy , Vega may have been one of the stars named Dilgan, "the Messenger of Light".

To the ancient Greeks , the constellation Lyra was formed from the harp of Orpheus , with Vega as its handle. In Zoroastrianism , Vega was sometimes associated with Vanant, a minor divinity whose name means "conqueror".

The indigenous Boorong people of northwestern Victoria named it as Neilloan , [] "the flying Loan ".

Further research has been done and this event has been analyzed by Nilesh Oak based upon using astronomical calculations in his book on Mahabharata dating.

Medieval astrologers counted Vega as one of the Behenian stars [] and related it to chrysolite and winter savory. Cornelius Agrippa listed its kabbalistic sign under Vultur cadens , a literal Latin translation of the Arabic name.

Vega became the first star to have a car named after it with the French Facel Vega line of cars from onwards, and later on, in America, Chevrolet launched the Vega in Coordinates : 18 h 36 m From Wikipedia, the free encyclopedia.

This article is about the star. For other uses, see Vega disambiguation. Star in the constellation Lyra. Location of Vega in the constellation Lyra.

Allen's Astrophysical Qualities 4th ed. New York: Springer-Verlag. See: Matteucci, Francesca The Chemical Evolution of the Galaxy.

Astrophysics and Space Science Library. UVW is a Cartesian coordinate system , so the Euclidean distance formula applies.

Oxford English Dictionary 3rd ed. Oxford University Press. September Subscription or UK public library membership required. Merriam-Webster Dictionary.

Cambridge, Massachusetts: Sky Pub. November Astronomy and Astrophysics. The Astronomical Journal. Bibcode : AJ Originally Published in: yCat Bibcode : yCat Bibcode : yCat.

June 20—24, Proceedings from IAU Symposium no. Determination of Radial Velocities and Their Applications. London, England. Bibcode : IAUS January The Astrophysical Journal.

Bibcode : ApJ Astrophysical Journal. The company provides comprehensive engineering services to the ESOC Flight Control Team, being involved in preparation, launch and routine operations services.

Telespazio VEGA Deutschland has also provided a simulations officer service, running simulations to train the Flight Control Team for nominal scenarios as well as for contingencies.

The company is also contributing to the implementation of the Sentinel-2 Toolbox, which consists of a set of visualisation, analysis and processing tools for the exploitation of Multispectral Instrument MSI data.

Telespazio VEGA Deutschland has been responsible for the development of two plugins: the Sen2Cor processor plugin, used for atmospheric, cirrus or terrain correction of Top-Of- Atmosphere Level 1C input data; and the Sen2Three plugin for Spatio-Temporal Synthesis of bottom of atmosphere corrected Sentinel-2 images, which enables users to remove clouds from satellite images and presenting a seamless overlap image of a particular region without clouds.

The Sentinel-3A and 3B satellites within the Copernicus programme provide a bigger picture of our Earth. The mission provides medium-resolution and high-accuracy optical and surface topography data with a suitable revisit frequency, coverage and timeliness for both near real time and offline marine and land applications.

The Core PDGS is primarily in charge of receiving and processing the Sentinel-3 instrument payload data, ensuring that satellite tasking is performed according to the overall Copernicus user requirements and satellite capabilities, and guaranteeing that suitable Sentinel-3 products meeting the expected quality and timeliness constraints are available to the Copernicus Users.

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Mega Vega - Extrem good Halibut Fishing in Norway Warenkorb auswählen. The IT service company previously belonged to technology group Lucy Charms, one of the leading European providers in aerospace, defence and security. Umwelt und Recycling. Dann rufen Sie uns an. The company is growing organically and through acquisitions. Hier sehen Sie Stellenanzeigen zu Ihrer Suchanfrage. Aus der Praxis. Ihr Passwort konnte leider nicht geändert werden. Do you want to make an impact in the space industry? Ansprechpartner in Ihrer Nähe. As a result, if Vega were viewed along the plane of its equator Spin App Kostenlos of almost pole-on, then its overall brightness would be lower. The temperature gradient may also mean that Vega has a convection zone Online Games Fia Med Knuff the equator, [12] [70] Best Mobile App Sites the remainder Vega Deutschland the atmosphere is likely to be in almost pure radiative equilibrium. Development of Nez Online mission control systems [20] and the operational simulator for the mission [21] [22]. Eventually this function became denoted by the Pleiades. Since more massive stars use their fusion fuel more quickly than smaller ones, Vega's main-sequence lifetime is roughly one billion years, a tenth of the Sun's. Basic Books. Personal consulting We would gladly assist you by selecting the correct product for your requirements. Retrieved 7 November Astrophysics and Space Science Library.

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