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The Nature of Science
The Nature of Science

... dating, which is used to determine the ages of rocks  The oldest rocks found anywhere in the solar system are meteorites, the bits of meteoroids that survive passing through the Earth’s atmosphere and land on our planet’s surface  Radioactive age-dating of meteorites, reveals that they are all nea ...
The Nature of Science
The Nature of Science

... dating, which is used to determine the ages of rocks  The oldest rocks found anywhere in the solar system are meteorites, the bits of meteoroids that survive passing through the Earth’s atmosphere and land on our planet’s surface  Radioactive age-dating of meteorites, reveals that they are all nea ...
Dark Matter -24-------------------------------~-----------R-E-S-O-N-A-N-C
Dark Matter -24-------------------------------~-----------R-E-S-O-N-A-N-C

... There have been three reactions to the discovery of dark matter: (i) It doesn't exist; the law of gravitation must be modified so that the stars are all there is to a galaxy. (ii) Dark matter exists, but consists entirely of ord~nary matter - Jupiter-like objects called broum dwarfs that are not mas ...
Herschel
Herschel

... the Solar System placed beyond the orbit of Neptune (30 UA) up to ~55 UA. It is similar to the asteroid belt but 20 times wider and 20-200 times more massive. ...
The substance of gravity
The substance of gravity

... dark. However, a second look at the renowned diffraction experiment, where two coherent rays of light combine with each other to produce a pattern of bright and dark fringes, suggests to us that at a dark fringe electromagnetic fields do indeed cancel each other, but the quanta of light themselves, ...
In Search of the Dark Matter in the Universe
In Search of the Dark Matter in the Universe

... would be roughly the equivalent of 10 hydrogen atoms per cubic meter. This seems incredibly small, like a vacuum, when compared to the density of our earth and planets, but seen on a cosmic scale it represents a lot of matter. ...
Here`s
Here`s

... object appears brighter for a short time. Astronomers search for MACHOs (usually brown dwarfs) in the halo of our galaxy by monitoring the brightness of stars near the center of our galaxy and of stars in the Large Magellanic Cloud. The MACHO Project, one of the groups using this "gravitational len ...
The First Stars in the Universe
The First Stars in the Universe

... universe of 13.7 billion years). Researchers will need better telescopes to see more distant objects dating from still earlier times. Cosmologists, however, can make deductions about the early universe based on the cosmic microwave background radiation, which was emitted about 400,000 years after th ...
Relocation Diffusion
Relocation Diffusion

... One inch represents one mile conveys more meaning than 1:63,630. Used little in places where people use metric system. People familiar with centimeters and kilometers have little need for verbal scales to tell them that 1:100,000 means that one centimeter equals 1 kilometer or that 1:250,000 means t ...
Steven R. Majewski - UCLA Physics & Astronomy
Steven R. Majewski - UCLA Physics & Astronomy

... • But numerous problems matching data on galaxy scales, e.g.: – “missing satellites problem”/mass spectrum of subhalos – “central cusps problem” – “angular momentum problems” Abadi et al. (2003): “Current cosmological simulations have difficulties making anything that looks like a real galaxy.” ...
25.4 Galaxies and the Universe
25.4 Galaxies and the Universe

... • The Milky Way arch emerging from the Cerro Paranal, Chile, on the left, and sinking into the Antofagasta's night lights. The bright object in the center, above the Milky Way is Jupiter, somehow elongated due to the panoramic projection. The Magellanic Clouds are visible on the left side, and a pla ...
Lecture
Lecture

... Universe has been expanding at a constant rate since the beginning. – However, the gravity of objects will tend to slow the expansion over time (deceleration). – On the other hand, Einstein’s cosmological constant, if it exists, could cause the expansion to ...
Eyeing the retina nebula
Eyeing the retina nebula

... Planetary nebulae play a key role in recycling these materials throughout the universe. Without them rocky planets like the Earth and carbon-based life forms like us would not exist. The image of the Retina Nebula has been enhanced to dramatize its beauty. The difference in brightness between the ce ...
Cosmological Aspects of Nucleosynthesis
Cosmological Aspects of Nucleosynthesis

... Implication of the discovery of SN2007 bi  The estimated high core mass is in conflict with the commonly used mass loss rates as a function of metallicity  Regardless the correct description of mass loss, the data indicate that an extremely massive stars (>150 Msun ) are formed in the local unive ...
The Milky Way Galaxy
The Milky Way Galaxy

... Just as black holes and other massive objects curve space around them, galaxies and galaxy clusters curve space. When the alignment of a large mass and background objects is right, a dramatic effect is observed. This is known as a gravitational lens. ...
The Planets
The Planets

... can reach temperatures around 700 degrees Fahrenheit, while the side away from the Sun has temperatures of about -330 degrees Fahrenheit. Venus has thick clouds of sulfur that trap the Sun’s heat and make it the hottest planet in the Solar System. It also rotates in the opposite direction as most of ...
Section 7 The Big Bang Theory
Section 7 The Big Bang Theory

Warm- up Question Tell me what you know about The Big Bang
Warm- up Question Tell me what you know about The Big Bang

... Gravity and Fusion cause solar materials to constantly rise and fall Gas also moves because of the solar rotation The equator rotates in 25.3 days The poles in 33 days Average is 27 days ...
Larger, high-res file, best for printing
Larger, high-res file, best for printing

... reaches it. The spacecraft is equipped with seven different instrubreakthrough came in 1978, when James Christy discovered that ments, including a telescopic camera that will show us for the first Pluto has a satellite, soon named Charon. This made it possible to time what Pluto’s surface looks like ...
PDF
PDF

... Eric Høg in his 2001 Miraculous approval of Hipparcos, the key idea of using slits and photo cells to measure the position and brightness of stars as they pass in front of a detector, was posed first in 1926 by B. Strömgren. Høg himself in 1960 extended the idea by including counting techniques that ...
Power Point Presentation
Power Point Presentation

... and evolution (F. Zuccarello) (4) Magnetic helicity transport: We investigated the magnetic helicity balance in an active region where a confined solar eruption occurred. This was done in order to verify a possible relationship between the filament expansion and the helicity transport at its footpoi ...
The Hidden Lives of Galaxies NSTA 2001
The Hidden Lives of Galaxies NSTA 2001

... elliptical. Stars form within initial distribution of gas,and follow their initial orbits. - If stars form later, the gas has time to collapse into a disk. Most stars from within the disk. The galaxy becomes a spiral. ...
page proofs
page proofs

... In parallel to the experimental work of Shapley, Hubble and other astronomers, theoretical physics was making tremendous progress. In particular, Albert Einstein published his General Theory of Relativity in 1915, which provided a new way of understanding gravity. Until then, scientists had used Isa ...
Astronomy - Core Knowledge Foundation
Astronomy - Core Knowledge Foundation

... (Sadler, 1987). At this early grade level, students are  help to reinforce and extend learning about the  not expected to explain the seasons or the cause of  nature of light and the sun.  the phases of the moon Instead, they will be focusing  on the development of key terms and language that  Misco ...
here - Stars `r` Us!
here - Stars `r` Us!

... he title of this article needs some explanation. Clearly, the universe is not entirely made of molecules and we are exaggerating. In fact, most of the mass in the universe is probably not even made of familiar matter, i.e. the atoms and molecules of which we, the Earth, the solar system, and all the ...
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Outer space



Outer space, or just space, is the void that exists between celestial bodies, including the Earth. It is not completely empty, but consists of a hard vacuum containing a low density of particles, predominantly a plasma of hydrogen and helium as well as electromagnetic radiation, magnetic fields, neutrinos, dust and cosmic rays. The baseline temperature, as set by the background radiation from the Big Bang, is 2.7 kelvin (K). Plasma with a number density of less than one hydrogen atom per cubic metre and a temperature of millions of kelvin in the space between galaxies accounts for most of the baryonic (ordinary) matter in outer space; local concentrations have condensed into stars and galaxies. In most galaxies, observations provide evidence that 90% of the mass is in an unknown form, called dark matter, which interacts with other matter through gravitational but not electromagnetic forces. Data indicates that the majority of the mass-energy in the observable Universe is a poorly understood vacuum energy of space which astronomers label dark energy. Intergalactic space takes up most of the volume of the Universe, but even galaxies and star systems consist almost entirely of empty space.There is no firm boundary where space begins. However the Kármán line, at an altitude of 100 km (62 mi) above sea level, is conventionally used as the start of outer space in space treaties and for aerospace records keeping. The framework for international space law was established by the Outer Space Treaty, which was passed by the United Nations in 1967. This treaty precludes any claims of national sovereignty and permits all states to freely explore outer space. Despite the drafting of UN resolutions for the peaceful uses of outer space, anti-satellite weapons have been tested in Earth orbit.Humans began the physical exploration of space during the 20th century with the advent of high-altitude balloon flights, followed by manned rocket launches. Earth orbit was first achieved by Yuri Gagarin of the Soviet Union in 1961 and unmanned spacecraft have since reached all of the known planets in the Solar System. Due to the high cost of getting into space, manned spaceflight has been limited to low Earth orbit and the Moon.Outer space represents a challenging environment for human exploration because of the dual hazards of vacuum and radiation. Microgravity also has a negative effect on human physiology that causes both muscle atrophy and bone loss. In addition to these health and environmental issues, the economic cost of putting objects, including humans, into space is high.
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