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The Formation of the Solar System
The Formation of the Solar System

Point-like source searches with ANTARES
Point-like source searches with ANTARES

... weighed by the number of events in the data sample. ...
Look Up – Look Waaaaay Up!
Look Up – Look Waaaaay Up!

... controlled sense of wonder before the universal mystery, whether it hides in a snail's eye or within the light that impinges on that delicate organ. The second kind of observer is the extreme reductionist who is so busy stripping things apart that the tremendous mystery has been reduced to a trifle, ...
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NEW PARTICLES FROM NUCLEAR REACTIONS IN THE SUN Max

... one can set limits on their possible existence, or perhaps find evidence for it, by cosmological or astrophysical arguments [ 1]. Such particles would be produced in large numbers from the thermal energy in the interior of stars. Limits on the particle's properties may be set by the requirement that ...
Cosmology:
Cosmology:

... Theories describe a complex set of events and are true and revisable as technology develops. Laws explain simple universal happenings like gravity. 3. True or False: The best way to describe the universe or unknown is to observe what happens on Earth and apply that knowledge elsewhere. 4. The Univer ...
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Classroom activity

Neutrinos in an Expanding Universe Paper (IOP)
Neutrinos in an Expanding Universe Paper (IOP)

... Since neutrinos are subject to gravitational forces, their spectra were affected by this developing nonuniformity. The neutrino velocities either increased or decreased as a result of gravitational acceleration or deceleration, depending on the direction of motion of the particles with respect to th ...
Chapter 12: Stellar Evolution  - Otto
Chapter 12: Stellar Evolution - Otto

... End Points of Evolution for Stars of Different ...
Nova Scotia Grade One Earth and Space Science: Daily and
Nova Scotia Grade One Earth and Space Science: Daily and

Indirect Observation Method - Portal do Professor
Indirect Observation Method - Portal do Professor

... subjective reality of the observer can lead to different procedures and result in a different “objective” reality for the observer. This curious phenomenon has been observed in the most diverse scientific fields, such as quantum physics, in which a physical entity can behave as a wave when no one is ...
Binary Star Par 1802 Word Document
Binary Star Par 1802 Word Document

... which throws up questions. It consists of two young stars which have not yet reached the main sequence (i.e. they haven’t settled down into a stable hydrogen-burning state) and each have about 40% of the Sun’s mass. They apparently formed together about 1 million years ago. Their radii are approxima ...
Size and Scale
Size and Scale

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fall semester review

... 35. If a star is 17 light years away from us, how long does it take light from that star to reach Earth? 17 years 36. What is the importance of using different units of measurement for different lengths? Some distances are much shorter or longer than others so we use different measurements to make ...
PHYS 2410 General Astronomy Homework 7
PHYS 2410 General Astronomy Homework 7

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Lecture 7

The Sun and the Stars
The Sun and the Stars

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OUR UNIVERSE Problem Set 7 Solutions Question A1 Question A2

... (a) The hydrogen-burning main sequence phase, As the proto-star collapses under its own gravity its atoms (hydrogen about 70 % and helium about 25 %) heat up because they exchange gravitational potential energy for kinetic energy, eventually the atoms in the core reach temperatures of about 15 milli ...
Homework 1
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... sample of radioactive material under different environmental conditions. The sample is divided into four identical parts and placed within identical apparatus to measure the decay rates. The following experiments are performed: a) at standard temperature an pressure in the laboratory b) at high atmo ...
The Origin of Oxygen Isotopic Anomalies Seen in Primitive Meteorites
The Origin of Oxygen Isotopic Anomalies Seen in Primitive Meteorites

Lecture 9
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... We now need to assume something about the source of pressure in the star.  We require an equation of state to relate the pressure to macroscopic properties of the gas (i.e. temperature and density) ...
Slide 1
Slide 1

... Between thirty and fifty percent of all stars in the night sky belong to binary, or double star, systems. Under the right conditions, binary systems can enter stages of evolution that do not occur for single stars. One particularly interesting example is known as a common envelope (CE) phase, during ...
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For a big view of inner Earth, catch a few

Scientists Find Possible Birth of Tiniest Known Solar System ?
Scientists Find Possible Birth of Tiniest Known Solar System ?

... • "Our goal is to determine the smallest 'sun' with evidence for planet formation," said Luhman. "Here we have a sun that is so small it is the size of a planet. The question then becomes, what do we call any little bodies that might be born from this disk: planets or moons?“ • If this proto-planet ...
File - Prairie Science
File - Prairie Science

... cosmic "big bang" that began the universe some 10 billion to 20 billion years ago. In the milliseconds following this explosion, clouds of gases began to coalesce, collapse, and compress under gravity to form the building blocks of galaxies. ...
MSci Astrophysics 210PHY412
MSci Astrophysics 210PHY412

... Method of energy transport There are three ways energy can be transported in stars • Convection – energy transport by mass motions of the gas • Conduction – by exchange of energy during collisions of gas particles (usually e-) • Radiation – energy transport by the emission and absorption of photons ...
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Standard solar model

The standard solar model (SSM) is a mathematical treatment of the Sun as a spherical ball of gas (in varying states of ionisation, with the hydrogen in the deep interior being a completely ionised plasma). This model, technically the spherically symmetric quasi-static model of a star, has stellar structure described by several differential equations derived from basic physical principles. The model is constrained by boundary conditions, namely the luminosity, radius, age and composition of the Sun, which are well determined. The age of the Sun cannot be measured directly; one way to estimate it is from the age of the oldest meteorites, and models of the evolution of the Solar System. The composition in the photosphere of the modern-day Sun, by mass, is 74.9% hydrogen and 23.8% helium. All heavier elements, called metals in astronomy, account for less than 2 percent of the mass. The SSM is used to test the validity of stellar evolution theory. In fact, the only way to determine the two free parameters of the stellar evolution model, the helium abundance and the mixing length parameter (used to model convection in the Sun), are to adjust the SSM to ""fit"" the observed Sun.
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