Planetas exteriores final.pptx 6 a blog
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Jupiter is the largest planet in the solar system. It takes 12 years to orbit the sun but only 9 hours to rotate on its axis. Jupiter has rings composed of dust and a massive storm that has been raging for over 300 years. The document also mentions Jovian compounds, which refers to elements and chemicals common on Jupiter.
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The document discusses Earth's place in the universe and its early atmosphere. It describes how the Big Bang theory led to the formation of galaxies, stars and planets around 12-14 billion years ago. A supernova 7 billion years ago helped form a solar nebula that collapsed to create our sun and planets like Earth. Earth was initially a molten ball surrounded by hydrogen and helium. Volcanic activity produced an early atmosphere lacking in oxygen. Photosynthesis by early organisms introduced oxygen and led to the evolution of more complex life on Earth.
Solar System Formation/Sun/Comets/Meteors
The document summarizes theories about how our solar system formed from a collapsing cloud of gas and dust. It describes how:
1) Our solar system likely began from a giant interstellar cloud that collapsed under gravity and formed a rotating disk, with a dense center that became the Sun and a surrounding disk that formed the planets.
2) The solar nebula disk varied in temperature by distance from the Sun, allowing different elements to condense into planetary cores near and far from the Sun, forming the terrestrial and gas giant planets.
3) Asteroids and comets are remnants from solar system formation and provide clues about its early history through observations and analysis of their composition and orbits.
Formation ofthe solar system notes
The formation of the solar system began from a large cloud of gas and dust called the solar nebula. As the nebula collapsed due to gravity, it formed a disc with the sun at the center. Planetesimals within the disc collided and accreted to form the planets. The nebular theory explained many characteristics of the solar system but did not account for all observations. The modern condensation theory expanded on this model and better explained features such as the asteroid belt and comets through processes like condensation and fractionation within the early solar system.
Jupiter
Jupiter is the 5th planet from the sun and the largest planet in our solar system, taking just under 10 hours to complete one rotation. It has 64 known moons and is surrounded by a system of thin rings. Jupiter is so large that all the other planets in our solar system could fit inside of it.
What is in space
The document provides information about various celestial objects in space, including planets in our solar system (Venus, Earth, Mars, Jupiter, Saturn, Uranus, Neptune, Pluto), comets, meteors, stars, black holes, asteroids, galaxies, constellations, and our sun and moon. It describes characteristics of each object such as their composition, size, position from the sun, appearance, and other distinguishing features. The information is presented briefly in simple terms appropriate for elementary school students.
05 (may) 5 & 6 16.3c the solar system - formation
According to geological evidence, the solar system formed approximately 4.6 billion years ago from a large cloud of dust and gas that collapsed due to gravity. A disk formed with the sun at the center, and planets formed farther out from the accretion of smaller particles that collided and stuck together. The locations and motions of the planets can be explained by this process, with gas giants forming farther out due to radiation pressure and terrestrial planets closer due to gravity. The moon's surface is covered in impact craters from asteroids early in the solar system's history and contains dark lava seas.
Earth
This presentation explaining about Earth in General, Description of earth and several fact of earth . May it useful for all the reader:) don't forget to send your slide share too, i'll wait. Please Welcome..
Natural sciences presentation
an insight into how our universe was initially started and how each feature has such significance in the balance on the life on earth.
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The document discusses Earth's place in the universe and its early atmosphere. It describes how the Big Bang theory led to the formation of galaxies, stars and planets around 12-14 billion years ago. A supernova 7 billion years ago helped form a solar nebula that collapsed to create our sun and planets like Earth. Earth was initially a molten ball surrounded by hydrogen and helium. Volcanic activity produced an early atmosphere lacking in oxygen. Photosynthesis by early organisms introduced oxygen and led to the evolution of more complex life on Earth.
Solar System Formation/Sun/Comets/Meteors
The document summarizes theories about how our solar system formed from a collapsing cloud of gas and dust. It describes how:
1) Our solar system likely began from a giant interstellar cloud that collapsed under gravity and formed a rotating disk, with a dense center that became the Sun and a surrounding disk that formed the planets.
2) The solar nebula disk varied in temperature by distance from the Sun, allowing different elements to condense into planetary cores near and far from the Sun, forming the terrestrial and gas giant planets.
3) Asteroids and comets are remnants from solar system formation and provide clues about its early history through observations and analysis of their composition and orbits.
Formation ofthe solar system notes
The formation of the solar system began from a large cloud of gas and dust called the solar nebula. As the nebula collapsed due to gravity, it formed a disc with the sun at the center. Planetesimals within the disc collided and accreted to form the planets. The nebular theory explained many characteristics of the solar system but did not account for all observations. The modern condensation theory expanded on this model and better explained features such as the asteroid belt and comets through processes like condensation and fractionation within the early solar system.
Jupiter
Jupiter is the 5th planet from the sun and the largest planet in our solar system, taking just under 10 hours to complete one rotation. It has 64 known moons and is surrounded by a system of thin rings. Jupiter is so large that all the other planets in our solar system could fit inside of it.
What is in space
The document provides information about various celestial objects in space, including planets in our solar system (Venus, Earth, Mars, Jupiter, Saturn, Uranus, Neptune, Pluto), comets, meteors, stars, black holes, asteroids, galaxies, constellations, and our sun and moon. It describes characteristics of each object such as their composition, size, position from the sun, appearance, and other distinguishing features. The information is presented briefly in simple terms appropriate for elementary school students.
05 (may) 5 & 6 16.3c the solar system - formation
According to geological evidence, the solar system formed approximately 4.6 billion years ago from a large cloud of dust and gas that collapsed due to gravity. A disk formed with the sun at the center, and planets formed farther out from the accretion of smaller particles that collided and stuck together. The locations and motions of the planets can be explained by this process, with gas giants forming farther out due to radiation pressure and terrestrial planets closer due to gravity. The moon's surface is covered in impact craters from asteroids early in the solar system's history and contains dark lava seas.
Earth
This presentation explaining about Earth in General, Description of earth and several fact of earth . May it useful for all the reader:) don't forget to send your slide share too, i'll wait. Please Welcome..
Natural sciences presentation
an insight into how our universe was initially started and how each feature has such significance in the balance on the life on earth.
Solar system formation[1]
The document summarizes the Nebular Theory of solar system formation. It states that the solar system formed from a rotating cloud of gas and dust remnants from a supernova. As the cloud collapsed under gravity, it flattened into a disc and spun faster. The center became very hot and formed the Sun, while the planets formed from accretion of planetesimals in the disc. The terrestrial planets are rocky, while the gas giants formed from condensation of ices and gases in the outer solar system. However, some observations of exoplanets do not fully match this theory.
Universe and Solar System
Here are my thoughts on your questions:
1. It seems highly probable that there are other life forms exploring the universe besides humans. The universe is immense, with billions of galaxies and trillions of planets. Given these vast numbers, it would be surprising if life did not arise elsewhere. However, the distances involved are also immense, so contact with other civilizations may not occur for a very long time, if ever.
2. The expansion of the universe is occurring at the scale of galaxies and galaxy clusters - it does not affect smaller scales like the Earth-Sun distance. Gravity between the Earth and Sun is strong enough to overcome any tiny effects from the universe's expansion. So the increasing distance between galaxies will not directly
Origins of Our Solar System
The solar system formed from a giant cloud of dust and gas called a nebula approximately 5 billion years ago. As the nebula collapsed due to gravity, the densest parts compressed at its center to form the proto-Sun, while the remaining material flattened into a disk that would eventually form the planets. Over millions of years, dust particles in the disk collided and stuck together, growing into ever larger bodies including planets that began to orbit the newborn Sun. The inner terrestrial planets closest to the Sun include Mercury, Venus, Earth, and Mars, while the outer gas giants are Jupiter, Saturn, Uranus, and Neptune. In a few billion years, the Sun will grow hotter and expand, likely consuming the inner planets
I. a. universe and solar system
This document discusses theories of the formation of the universe and solar system according to Earth science. It describes the Big Bang theory, which proposes that the universe began from an explosion of dense matter around 13.8 billion years ago, as supported by evidence from cosmic microwave background radiation. It also discusses the cosmic inflation theory of rapid early expansion, and the steady state theory of a constantly expanding universe without a beginning. Regarding solar system formation, it outlines the nebular hypothesis of planets forming from a rotating gas disk around the young Sun, and the planetesimal and tidal theories involving accumulation of small planetary bodies.
Comets
Comets originate far from the Sun and have highly elliptical orbits that bring them close to the Sun periodically. A comet is composed of dust and frozen gases like water, carbon dioxide and methane. When a comet approaches the Sun, its frozen gases heat and vaporize, forming an atmosphere around the comet's icy nucleus and two distinct tails - a curved dust tail and a straight ion tail that can be as long as Earth's orbit. Recent missions like Rosetta have provided images of bizarrely shaped comet nuclei and clues about their young, evolving surfaces from emitted jets and circular pits.
Antonio
The document discusses the structure and history of the universe according to cosmological theories. It describes how the universe began as a hot dense plasma following the Big Bang around 13 billion years ago. It formed into hydrogen and helium gases which later coalesced into the first stars and galaxies. The universe is still expanding today due to the initial force of the Big Bang and dark energy. The document also examines theories about different astronomical objects like galaxies, nebulae, quasars, black holes and planetary systems.
Space
The document discusses facts about space exploration and celestial bodies. It notes that the first, current, and third millennia consist of different numbers of days due to the calendar system used. It also mentions that the Space Age began on October 4, 1957 and that the first woman in space was Russian Valentina Tereshkova. Additionally, it provides various facts about planets such as Venus rotating clockwise and Olympus Mons being the largest volcano in the solar system.
Our solar system book
The document is a 1,766 word informational text about the solar system from the website Reading A-Z. It provides descriptions of the sun, eight official planets (Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus, Neptune), dwarf planets like Pluto, asteroids, comets, and other objects in the solar system. It includes illustrations and photographs to accompany the written descriptions of each celestial body.
Formation of the Solar System
The document provides information on the formation of the solar system. It describes the two categories of planets - terrestrial planets which are closest to the sun and include Mercury, Venus, Earth, and Mars, and jovian planets which are gas giants including Jupiter, Saturn, Uranus, and Neptune. It then provides details on each of the planets, their physical characteristics such as size, composition and orbital properties. It also discusses other components of the solar system including asteroids, meteorites, comets, and the sun and moon.
The solar system - Phoenix University Guide
The document summarizes key information about the formation of the solar system and properties of planets in our solar system. It explains that the solar system formed from a giant cloud of gas and dust that collapsed under gravity around 4.6 billion years ago. It also provides details about the terrestrial planets like Earth, Mars, and Mercury including their geological features and atmospheric compositions. Visual aids like images and diagrams are included to supplement the textual information.
Solar system PPT
The document summarizes the key components of the solar system. It describes the terrestrial and Jovian planets, asteroids, meteoroids, and comets. It also outlines theories for how the solar system formed from an initial nebula of dust and gas, including how planets condensed from this nebula via accumulation of dust particles and subsequent collisions of planetesimals over hundreds of millions of years.
moon, mars, venus
The document provides information about the Moon:
- The Moon has 1/80 the mass and 1/4 the diameter of Earth. Its orbit is nearly circular with a mean distance of 384,000 km from Earth.
- The Moon causes Earth's tides and the slowing of Earth's rotation over time. The Moon's surface shows impact craters and lacks atmosphere or liquid water.
- Samples returned by Apollo astronauts show the Moon has a similar composition to Earth's mantle but is deficient in iron and volatiles like water, suggesting it formed from mantle material ejected during an ancient giant impact.
The origin of the solar system
The document discusses several scientific theories that explain the origin of the solar system. It begins by describing the nebular hypothesis proposed by Kant and Laplace, which suggests that the solar system formed from a cloud of gas and dust that collapsed under gravity. It then discusses the planetesimal and tidal theories which built upon this idea to explain how smaller planetesimals formed and were ejected from the sun. The protoplanet theory modified this view to incorporate modern knowledge about independent formation of matter in protoplanets within the rotating nebula.
Earth
Earth began forming over 4.6 billion years ago from a cloud of gas and dust that also formed the Sun and other planets. As the solar system developed, small objects called planetesimals collided and stuck together, eventually forming Earth. When Earth first formed, it was a hot molten planet bombarded by asteroids and comets. As it cooled over millions of years, the first life forms of bacteria emerged and the oceans and atmosphere developed. Today, Earth is a complex system made up of interacting spheres including the atmosphere, biosphere, geosphere, hydrosphere, and cryosphere that sustain life.
Solar system
This document provides an overview of the solar system, including its origin, components, and current state of study. It describes the sun and planets Mercury through Neptune. It also discusses dwarf planets, satellites or moons, asteroids, and comets. The solar system formed from a solar nebula according to the nebular hypothesis. Today, the solar system is studied using land and space-based telescopes as well as space missions.
Solar system and earth
Presentation about what is solar system and earth , how both these are formed and evloved through out the time
I.A Universe and Solar system
The document summarizes the origin and structure of the Earth and solar system. It describes theories for the formation of the universe like the Big Bang theory and theories for the formation of the solar system. It then describes the structure and components of the solar system including the inner terrestrial planets like Earth and Mars, outer gas giants like Jupiter and Saturn, and other minor objects like asteroids, comets, and meteorites. It provides details on the composition, atmospheres, moons, and other features of each planet and minor solar system member.
History of our solar system
The document summarizes how the planets in our solar system formed. It explains that the sun and planets originated from a large cloud of gas and dust that collapsed under gravity around 10-20 billion years ago. As the cloud collapsed, it formed a disk and the planets developed from this disk of gas and dust. The inner planets Mercury, Venus, Earth and Mars formed close to the sun from this nebula, while the outer gas giants Jupiter, Saturn, Uranus and Neptune formed farther from the sun where it was cooler and ice could form.
Science blog
Stars are spheres of gas where nuclear reactions produce light and heat. They are classified by color, size, and luminosity. Constellations are groups of stars that are easily identified from Earth and are named by their shape. Galaxies are enormous systems of stars, dust and gas held together by gravity, and they are divided into spiral, elliptical, and irregular galaxies. Our solar system is located in the Milky Way galaxy.
Science blog
Stars are spheres of gas where nuclear reactions produce light and heat. They are classified by color, size, and luminosity. Constellations are groups of stars that are easily identified from Earth and are named by their shape. Galaxies are enormous systems of stars, dust and gas held together by gravity that are divided into spiral, elliptical, and irregular galaxies. Our solar system is located in the Milky Way galaxy.
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Solar system formation[1]
The document summarizes the Nebular Theory of solar system formation. It states that the solar system formed from a rotating cloud of gas and dust remnants from a supernova. As the cloud collapsed under gravity, it flattened into a disc and spun faster. The center became very hot and formed the Sun, while the planets formed from accretion of planetesimals in the disc. The terrestrial planets are rocky, while the gas giants formed from condensation of ices and gases in the outer solar system. However, some observations of exoplanets do not fully match this theory.
Universe and Solar System
Here are my thoughts on your questions:
1. It seems highly probable that there are other life forms exploring the universe besides humans. The universe is immense, with billions of galaxies and trillions of planets. Given these vast numbers, it would be surprising if life did not arise elsewhere. However, the distances involved are also immense, so contact with other civilizations may not occur for a very long time, if ever.
2. The expansion of the universe is occurring at the scale of galaxies and galaxy clusters - it does not affect smaller scales like the Earth-Sun distance. Gravity between the Earth and Sun is strong enough to overcome any tiny effects from the universe's expansion. So the increasing distance between galaxies will not directly
Origins of Our Solar System
The solar system formed from a giant cloud of dust and gas called a nebula approximately 5 billion years ago. As the nebula collapsed due to gravity, the densest parts compressed at its center to form the proto-Sun, while the remaining material flattened into a disk that would eventually form the planets. Over millions of years, dust particles in the disk collided and stuck together, growing into ever larger bodies including planets that began to orbit the newborn Sun. The inner terrestrial planets closest to the Sun include Mercury, Venus, Earth, and Mars, while the outer gas giants are Jupiter, Saturn, Uranus, and Neptune. In a few billion years, the Sun will grow hotter and expand, likely consuming the inner planets
I. a. universe and solar system
This document discusses theories of the formation of the universe and solar system according to Earth science. It describes the Big Bang theory, which proposes that the universe began from an explosion of dense matter around 13.8 billion years ago, as supported by evidence from cosmic microwave background radiation. It also discusses the cosmic inflation theory of rapid early expansion, and the steady state theory of a constantly expanding universe without a beginning. Regarding solar system formation, it outlines the nebular hypothesis of planets forming from a rotating gas disk around the young Sun, and the planetesimal and tidal theories involving accumulation of small planetary bodies.
Comets
Comets originate far from the Sun and have highly elliptical orbits that bring them close to the Sun periodically. A comet is composed of dust and frozen gases like water, carbon dioxide and methane. When a comet approaches the Sun, its frozen gases heat and vaporize, forming an atmosphere around the comet's icy nucleus and two distinct tails - a curved dust tail and a straight ion tail that can be as long as Earth's orbit. Recent missions like Rosetta have provided images of bizarrely shaped comet nuclei and clues about their young, evolving surfaces from emitted jets and circular pits.
Antonio
The document discusses the structure and history of the universe according to cosmological theories. It describes how the universe began as a hot dense plasma following the Big Bang around 13 billion years ago. It formed into hydrogen and helium gases which later coalesced into the first stars and galaxies. The universe is still expanding today due to the initial force of the Big Bang and dark energy. The document also examines theories about different astronomical objects like galaxies, nebulae, quasars, black holes and planetary systems.
Space
The document discusses facts about space exploration and celestial bodies. It notes that the first, current, and third millennia consist of different numbers of days due to the calendar system used. It also mentions that the Space Age began on October 4, 1957 and that the first woman in space was Russian Valentina Tereshkova. Additionally, it provides various facts about planets such as Venus rotating clockwise and Olympus Mons being the largest volcano in the solar system.
Our solar system book
The document is a 1,766 word informational text about the solar system from the website Reading A-Z. It provides descriptions of the sun, eight official planets (Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus, Neptune), dwarf planets like Pluto, asteroids, comets, and other objects in the solar system. It includes illustrations and photographs to accompany the written descriptions of each celestial body.
Formation of the Solar System
The document provides information on the formation of the solar system. It describes the two categories of planets - terrestrial planets which are closest to the sun and include Mercury, Venus, Earth, and Mars, and jovian planets which are gas giants including Jupiter, Saturn, Uranus, and Neptune. It then provides details on each of the planets, their physical characteristics such as size, composition and orbital properties. It also discusses other components of the solar system including asteroids, meteorites, comets, and the sun and moon.
The solar system - Phoenix University Guide
The document summarizes key information about the formation of the solar system and properties of planets in our solar system. It explains that the solar system formed from a giant cloud of gas and dust that collapsed under gravity around 4.6 billion years ago. It also provides details about the terrestrial planets like Earth, Mars, and Mercury including their geological features and atmospheric compositions. Visual aids like images and diagrams are included to supplement the textual information.
Solar system PPT
The document summarizes the key components of the solar system. It describes the terrestrial and Jovian planets, asteroids, meteoroids, and comets. It also outlines theories for how the solar system formed from an initial nebula of dust and gas, including how planets condensed from this nebula via accumulation of dust particles and subsequent collisions of planetesimals over hundreds of millions of years.
moon, mars, venus
The document provides information about the Moon:
- The Moon has 1/80 the mass and 1/4 the diameter of Earth. Its orbit is nearly circular with a mean distance of 384,000 km from Earth.
- The Moon causes Earth's tides and the slowing of Earth's rotation over time. The Moon's surface shows impact craters and lacks atmosphere or liquid water.
- Samples returned by Apollo astronauts show the Moon has a similar composition to Earth's mantle but is deficient in iron and volatiles like water, suggesting it formed from mantle material ejected during an ancient giant impact.
The origin of the solar system
The document discusses several scientific theories that explain the origin of the solar system. It begins by describing the nebular hypothesis proposed by Kant and Laplace, which suggests that the solar system formed from a cloud of gas and dust that collapsed under gravity. It then discusses the planetesimal and tidal theories which built upon this idea to explain how smaller planetesimals formed and were ejected from the sun. The protoplanet theory modified this view to incorporate modern knowledge about independent formation of matter in protoplanets within the rotating nebula.
Earth
Earth began forming over 4.6 billion years ago from a cloud of gas and dust that also formed the Sun and other planets. As the solar system developed, small objects called planetesimals collided and stuck together, eventually forming Earth. When Earth first formed, it was a hot molten planet bombarded by asteroids and comets. As it cooled over millions of years, the first life forms of bacteria emerged and the oceans and atmosphere developed. Today, Earth is a complex system made up of interacting spheres including the atmosphere, biosphere, geosphere, hydrosphere, and cryosphere that sustain life.
Solar system
This document provides an overview of the solar system, including its origin, components, and current state of study. It describes the sun and planets Mercury through Neptune. It also discusses dwarf planets, satellites or moons, asteroids, and comets. The solar system formed from a solar nebula according to the nebular hypothesis. Today, the solar system is studied using land and space-based telescopes as well as space missions.
Solar system and earth
Presentation about what is solar system and earth , how both these are formed and evloved through out the time
I.A Universe and Solar system
The document summarizes the origin and structure of the Earth and solar system. It describes theories for the formation of the universe like the Big Bang theory and theories for the formation of the solar system. It then describes the structure and components of the solar system including the inner terrestrial planets like Earth and Mars, outer gas giants like Jupiter and Saturn, and other minor objects like asteroids, comets, and meteorites. It provides details on the composition, atmospheres, moons, and other features of each planet and minor solar system member.
History of our solar system
The document summarizes how the planets in our solar system formed. It explains that the sun and planets originated from a large cloud of gas and dust that collapsed under gravity around 10-20 billion years ago. As the cloud collapsed, it formed a disk and the planets developed from this disk of gas and dust. The inner planets Mercury, Venus, Earth and Mars formed close to the sun from this nebula, while the outer gas giants Jupiter, Saturn, Uranus and Neptune formed farther from the sun where it was cooler and ice could form.
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Stars are spheres of gas where nuclear reactions produce light and heat. They are classified by color, size, and luminosity. Constellations are groups of stars that are easily identified from Earth and are named by their shape. Galaxies are enormous systems of stars, dust and gas held together by gravity, and they are divided into spiral, elliptical, and irregular galaxies. Our solar system is located in the Milky Way galaxy.
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It is with great pleasure that we extend to you an invitation to the 5th Power Grid Model Meet-up, scheduled for 6th June 2024. This event will adopt a hybrid format, allowing participants to join us either through an online Mircosoft Teams session or in person at TU/e located at Den Dolech 2, Eindhoven, Netherlands. The meet-up will be hosted by Eindhoven University of Technology (TU/e), a research university specializing in engineering science & technology.
Power Grid Model
The global energy transition is placing new and unprecedented demands on Distribution System Operators (DSOs). Alongside upgrades to grid capacity, processes such as digitization, capacity optimization, and congestion management are becoming vital for delivering reliable services.
Power Grid Model is an open source project from Linux Foundation Energy and provides a calculation engine that is increasingly essential for DSOs. It offers a standards-based foundation enabling real-time power systems analysis, simulations of electrical power grids, and sophisticated what-if analysis. In addition, it enables in-depth studies and analysis of the electrical power grid’s behavior and performance. This comprehensive model incorporates essential factors such as power generation capacity, electrical losses, voltage levels, power flows, and system stability.
Power Grid Model is currently being applied in a wide variety of use cases, including grid planning, expansion, reliability, and congestion studies. It can also help in analyzing the impact of renewable energy integration, assessing the effects of disturbances or faults, and developing strategies for grid control and optimization.
What to expect
For the upcoming meetup we are organizing, we have an exciting lineup of activities planned:
-Insightful presentations covering two practical applications of the Power Grid Model.
-An update on the latest advancements in Power Grid -Model technology during the first and second quarters of 2024.
-An interactive brainstorming session to discuss and propose new feature requests.
-An opportunity to connect with fellow Power Grid Model enthusiasts and users.
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DLAU und die Lizenzen nach dem CCB- und CCX-Modell sind für viele in der HCL-Community seit letztem Jahr ein heißes Thema. Als Notes- oder Domino-Kunde haben Sie vielleicht mit unerwartet hohen Benutzerzahlen und Lizenzgebühren zu kämpfen. Sie fragen sich vielleicht, wie diese neue Art der Lizenzierung funktioniert und welchen Nutzen sie Ihnen bringt. Vor allem wollen Sie sicherlich Ihr Budget einhalten und Kosten sparen, wo immer möglich. Das verstehen wir und wir möchten Ihnen dabei helfen!
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