The Sun is our nearest star. It is a huge, luminous ball of gas like all the other stars. It consists mostly of hydrogen, and helium with tiny amounts of other elements. The Corona is the outer shell of the Sun’s atmosphere. It is extremely hot with temperatures reaching up to 2 million degrees. In the radiation zone, the energy is transported outwards by radiation. It covers about 70% of the Sun’s diameter.
The Sun
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The Sun Explained: Inside and Out
The Sun is the star at the focal point of the Earth's planetary group. It's just about splendidly round and comprises of blazing plasma entwined with attractive fields. It has a breadth of about 1,392,684 km, in the ballpark of 109 times that of Earth, and its mass (about 2×1030 kilograms, 330,000 times that of Earth) explains about 99.86% of the sum mass of the Sun oriented System. Synthet...
The Sun is the star at the focal point of the Earth's planetary group. It's just about splendidly round and comprises of blazing plasma entwined with attractive fields. It has a breadth of about 1,392,684 km, in the ballpark of 109 times that of Earth, and its mass (about 2×1030 kilograms, 330,000 times that of Earth) explains about 99.86% of the sum mass of the Sun oriented System. Synthet...
Other Solar Systems
Is our Solar system unique in the Universe ? Until recently, astronomers could only guess whether other stars are orbited by planetary systems. Extrasolar planets – those that orbit stars other than the Sun – are difficult to detect, because they are about one – billionth the brightness of their parent stars. Extrasolar planets can also be detected by watching for a drop in brightness as ...
Is our Solar system unique in the Universe ? Until recently, astronomers could only guess whether other stars are orbited by planetary systems. Extrasolar planets – those that orbit stars other than the Sun – are difficult to detect, because they are about one – billionth the brightness of their parent stars. Extrasolar planets can also be detected by watching for a drop in brightness as ...
Neptune Explained: Inside and Out
Neptune is the eighth and most distant planet from the Sun in the Earth's planetary group. It's the fourth-most expansive planet by distance across and the third-most vast by mass. Neptune is 17 times the mass of Earth and is to some degree more enormous than its close-twin Uranus, which is 15 times the mass of Earth but not as dense. On normal, Neptune circles the Sun at a separation of 30...
Neptune is the eighth and most distant planet from the Sun in the Earth's planetary group. It's the fourth-most expansive planet by distance across and the third-most vast by mass. Neptune is 17 times the mass of Earth and is to some degree more enormous than its close-twin Uranus, which is 15 times the mass of Earth but not as dense. On normal, Neptune circles the Sun at a separation of 30...
Deflecting Asteroids
Every object exerts a gravitational pull, including a single spacecraft. Merely by hovering above the asteroid. It could pull the rock off course. The approach could even be tried with the Dawn spacecraft, scheduled to finish its tasks in the asteroid belt by 2015. However, such a strategy would be very slow, requiring years or even decades to alter the path of the asteroid.
Every object exerts a gravitational pull, including a single spacecraft. Merely by hovering above the asteroid. It could pull the rock off course. The approach could even be tried with the Dawn spacecraft, scheduled to finish its tasks in the asteroid belt by 2015. However, such a strategy would be very slow, requiring years or even decades to alter the path of the asteroid.
Dwarf Planets Explained
After Pluto was discovered in 1930, it was regarded as the ninth major planet, although it was soon found to be very different from the others. It is smaller than Earth’s Moon and follows an elongated, titled orbit. In the 1990’s astronomers began to discover small bodies similar to Pluto beyond Neptune. Some, such as Eris, were larger then Pluto. In 2006, astronomers decided to define a ne...
After Pluto was discovered in 1930, it was regarded as the ninth major planet, although it was soon found to be very different from the others. It is smaller than Earth’s Moon and follows an elongated, titled orbit. In the 1990’s astronomers began to discover small bodies similar to Pluto beyond Neptune. Some, such as Eris, were larger then Pluto. In 2006, astronomers decided to define a ne...
Planetary System (GER)
A planetary framework is a situated of gravitationally bound non-stellar questions in circle around a star or star framework. Ordinarily vocalizing, planetary frameworks portray frameworks with one or more planets, admitting that such frameworks may additionally comprise of figures for example predominate planets, space rocks, expected satellites, meteoroids, comets and planetesimals and addit...
A planetary framework is a situated of gravitationally bound non-stellar questions in circle around a star or star framework. Ordinarily vocalizing, planetary frameworks portray frameworks with one or more planets, admitting that such frameworks may additionally comprise of figures for example predominate planets, space rocks, expected satellites, meteoroids, comets and planetesimals and addit...
What our Universe Looks Like From Another Universe
The universe is usually described as the totality of being, incorporating planets, stars, universes, the substance of intergalactic space, and all matter and energy. Definitions and regulation change and comparative terms incorporate the universe, the globe and nature. Exploratory perception of prior stages in the infrastructure of the universe, which could be perceived at paramount separates, pre...
The universe is usually described as the totality of being, incorporating planets, stars, universes, the substance of intergalactic space, and all matter and energy. Definitions and regulation change and comparative terms incorporate the universe, the globe and nature. Exploratory perception of prior stages in the infrastructure of the universe, which could be perceived at paramount separates, pre...
What are Exoplanets?
In 1543, Polish astronomer Nicolaus Copernicus published on the Revolutions of the Heavenly Spheres, showing that the Earth, far from being the privileged center of the universe, is just another planet orbiting the Sun. Since then, the discovery that our sun is a typical star among the billions in the Milky Way, which in turn is but one of the billions of galaxies we observe in all directions,...
In 1543, Polish astronomer Nicolaus Copernicus published on the Revolutions of the Heavenly Spheres, showing that the Earth, far from being the privileged center of the universe, is just another planet orbiting the Sun. Since then, the discovery that our sun is a typical star among the billions in the Milky Way, which in turn is but one of the billions of galaxies we observe in all directions,...
What Gravity does to Entropy
What qualifies as low entropy or high entropy depends on the situation. Physicists identify the high – entropy state of a system based on how the system evolves over time. For example, if a diffuse and sufficiently cool gas feels the tug of gravity, it evolves to a clump. The law of entropy increase then implies that the clump has high entropy, even though at first glance it might appear to be...
What qualifies as low entropy or high entropy depends on the situation. Physicists identify the high – entropy state of a system based on how the system evolves over time. For example, if a diffuse and sufficiently cool gas feels the tug of gravity, it evolves to a clump. The law of entropy increase then implies that the clump has high entropy, even though at first glance it might appear to be...
Fun Facts About the Space Shuttle
Finding out the length of an orbit is a very tedious task. Unless one have flown aboard the space shuttle or have seen it in person, it can be difficult to mentally visualize the size of the vehicle. Here, we measure the orbiter against a familiar object, a school bus. The weight of Orbiter would weight around 178000 pounds. The heaviest African Elephant weighs 13200 pounds. It would take appro...
Finding out the length of an orbit is a very tedious task. Unless one have flown aboard the space shuttle or have seen it in person, it can be difficult to mentally visualize the size of the vehicle. Here, we measure the orbiter against a familiar object, a school bus. The weight of Orbiter would weight around 178000 pounds. The heaviest African Elephant weighs 13200 pounds. It would take appro...
A Brief History of the Solar System
The process of existence or initiative of life in the Solar System looks very interesting. Life in the solar system is a monomeric nucleotide, pretty much just a simple molecular compound made out of a normal, every-day inorganic material. Life started in the Earth once the things inside it are cooled down a bit. Basically life in the Earth is a replicator, the way it just happened or formed. Life...
The process of existence or initiative of life in the Solar System looks very interesting. Life in the solar system is a monomeric nucleotide, pretty much just a simple molecular compound made out of a normal, every-day inorganic material. Life started in the Earth once the things inside it are cooled down a bit. Basically life in the Earth is a replicator, the way it just happened or formed. Life...
Is There an Edge of the Universe?
The “dark flow” of wayward galaxy clusters that appear to be pulled in one direction could give us our first hint of something beyond the cosmic horizon, which normally marks the limit of the observable universe.
The “dark flow” of wayward galaxy clusters that appear to be pulled in one direction could give us our first hint of something beyond the cosmic horizon, which normally marks the limit of the observable universe.
Mercury Explained: Inside and Out
Mercury is the deepest planet in the Earth's planetary group. It's additionally the most diminutive, and its circle is the most unconventional (that is, the slightest splendidly roundabout) of the eight planets. It circles the Sun once in the vicinity of 88 Earth days, finishing several revolutions about its hub for each two circles. The planet is named following the Roman god Mercury, the det...
Mercury is the deepest planet in the Earth's planetary group. It's additionally the most diminutive, and its circle is the most unconventional (that is, the slightest splendidly roundabout) of the eight planets. It circles the Sun once in the vicinity of 88 Earth days, finishing several revolutions about its hub for each two circles. The planet is named following the Roman god Mercury, the det...
Saturn and its Moons
Saturn is the sixth planet from the Sun and the second most expansive planet in the Earth's planetary group, following Jupiter. Named following the Roman god Saturn, its galactic image (♄) speaks for the god's sickle. Saturn is a gas mammoth with a middle range something like nine times that of Earth. While one and only one-eighth the mean thickness of Earth, with its more impressive volume Sa...
Saturn is the sixth planet from the Sun and the second most expansive planet in the Earth's planetary group, following Jupiter. Named following the Roman god Saturn, its galactic image (♄) speaks for the god's sickle. Saturn is a gas mammoth with a middle range something like nine times that of Earth. While one and only one-eighth the mean thickness of Earth, with its more impressive volume Sa...
Nearside of the Moon
The dominant features on the Moon’s nearside – the side that always faces the Earth – are the dark maria, which early astronomers thought were seas. These lava – filled basis formed when molten rock seeped through the Moon’s crust to fill depressions left by meteorite impacts.
The dominant features on the Moon’s nearside – the side that always faces the Earth – are the dark maria, which early astronomers thought were seas. These lava – filled basis formed when molten rock seeped through the Moon’s crust to fill depressions left by meteorite impacts.
National Geographic: The Heavens 1995
The movements in the Heavens are interminable and consummate, and the ideal movement is the round one, which, unlike the natural up-and down-ward headways, can final interminably similar. As substances, heavenly figures have matter (aether) and a shape: it appears that Aristotle did see them as living creatures with a reasonable soul as their shape.
The movements in the Heavens are interminable and consummate, and the ideal movement is the round one, which, unlike the natural up-and down-ward headways, can final interminably similar. As substances, heavenly figures have matter (aether) and a shape: it appears that Aristotle did see them as living creatures with a reasonable soul as their shape.
Debris That Hit Space Shuttles
There are many impacts of the Space Shuttle. Atlantis struck by debris from the nose cone of a solid rocket booster 85 seconds after liftoff causing 707 dents, 298 larger than one inch in diameter. Columbia Foam debris from the external tank causes more than 100 dents and spurs NASA to begin a program to resolve foam-shedding.
There are many impacts of the Space Shuttle. Atlantis struck by debris from the nose cone of a solid rocket booster 85 seconds after liftoff causing 707 dents, 298 larger than one inch in diameter. Columbia Foam debris from the external tank causes more than 100 dents and spurs NASA to begin a program to resolve foam-shedding.
NASA's Constellation Program Trips to the Moon
NASA’s Constellation program comprises a set of launch boosters, space vehicles and support modules that together will place humans on the moon by 2020. Plans call for astronauts to stay on the lunar surface for periods ranging from four days to more than six months.
NASA’s Constellation program comprises a set of launch boosters, space vehicles and support modules that together will place humans on the moon by 2020. Plans call for astronauts to stay on the lunar surface for periods ranging from four days to more than six months.
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