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what are stars made of?
what are stars made of?

PHYSICS 110: PHYSICS OF EVERYDAY PHENOMENA
PHYSICS 110: PHYSICS OF EVERYDAY PHENOMENA

apparent magnitude - Harding University
apparent magnitude - Harding University

... provided it is properly placed on the HR diagram. ...
Nebulas - WLWV Staff Blogs
Nebulas - WLWV Staff Blogs

... form between stars. They form in regions where gas, dust, and other materials clump together to create larger masses, which then gather other material until they become big enough to be known as stars. ...
“The Southern Cross”
“The Southern Cross”

... Aristotle’s world-view of a universe in which everything had its natural place with a changing Earth surrounded by eternal, perfect and incorruptible heavens was not seriously challenged for almost another two millennia when, in the 16th century, Copernicus contested the established acceptance of th ...
Planisphere
Planisphere

reach for the stars
reach for the stars

CO 2 Cycle
CO 2 Cycle

... carried sediment in the past several years…The atmosphere on Mars is so thin that liquid water cannot persist at the surface. However, researchers propose that water could remain liquid long enough, after breaking out from an underground source, to carry debris before totally evaporating and freezin ...
STEM for TY Teachers
STEM for TY Teachers

... !  Variable Stars - Stars that Vary in Luminosity: Many stars, even the Sun, can vary in luminosity. Some change their light output by a very significant amount in a regular way and can therefore be recognized at very great distances. These can be used as “standard candles” to estimate distances. ...
Binary Star - Armagh Observatory
Binary Star - Armagh Observatory

...  Eclipsing Binary: An eclipsing binary is two stars that appear to be a single star varying in brightness. The variation in brightness is due to the stars periodically obscuring or enhancing one another. Such binary star systems happen to be tilted (with respect to us) so that their orbital plane ...
Lesson one Time line Powerpoint
Lesson one Time line Powerpoint

... spheres in uniform (constant speed) and perfect, circular motions and earth was the center of motion (Geocentric). ...
Unit 8 Chapter 30
Unit 8 Chapter 30

... It is believed that stars probably formed in similar ways. The theory is that a cloud of dust (a nebula) contracts with most of the material going to the center to form a star. The dust is mainly Hydrogen (99%) with other elements and compounds like silicon carbide, graphite diamonds and nitrogen. T ...
Death of Low Mass Stars 8 Solar Masses or less
Death of Low Mass Stars 8 Solar Masses or less

... repulsion) keeps gravity from compressing it further. Called Electron Degeneracy • The black dwarf will continue to exist at temps close to absolute zero forever…. ...
Astronomy Activity: The Life-Line of the Stars
Astronomy Activity: The Life-Line of the Stars

... The brightness that a star has as seen from the Earth is called the apparent brightness . Stars which are very bright are called magnitude 1 stars . The next brightest are magnitude 2 stars. Then comes magnitude 3, 4, 5, and down to the very faintest stars visible with the naked eye, magnitude 6 sta ...
Spectroscopic Data
Spectroscopic Data

Document
Document

4th Grade Earth Science Unit Guide:
4th Grade Earth Science Unit Guide:

Patterns in the Night Sky
Patterns in the Night Sky

... A star map is a map of the night sky that shows the relative positions of the stars in a particular part of the sky (Figure 4). Some star maps show only those objects that can be seen with the unaided eye, while others show objects that can only be viewed using a telescope or other instrument. A sta ...
Astronomy and Space articles
Astronomy and Space articles

... by first looking for the three stars in a row in the constellation of Orion. These form Orion's belt, but they are also well known as the base of 'The Saucepan', formed from some of the stars of Orion. If you extend a line from the belt stars upwards and to the right, you will come across Sirius. Of ...
From Simulation to Visualization: Astrophysics Goes
From Simulation to Visualization: Astrophysics Goes

... Example: Earth orbiting the Sun ...
transparencies
transparencies

... E = M (ΔR/R)2 M mass in quadrupole motion For each mini-collapses ΔR/R ~ 2 – 3 × 10-3 E ~ 0.5 -1× 10-5 Solar masses (It can be one order of magnitude larger in more realistic calculations ) Four order of magnitude larger respect to SGR Energy scale of hadronic physics vs atomic nuclear physics ...
Measuring The Parallax of Barnard's Star
Measuring The Parallax of Barnard's Star

... established rate of proper motion of 10.37 arcseconds per year. And, the velocity in arcseconds per year times the distance in parsecs gives the velocity in astronomical units (au) per year. Using our derived numbers we get that the projected velocity is 19.3 au/yr. A natural question to ask is: why ...
Introduction to Astronomy
Introduction to Astronomy

... The weak nuclear force can change one type of subatomic particle into another in some situations such as radioactive decay, and the generation of energy in stars. The energy resulting from thermonuclear fusion is distributed in several ways: kinetic energy of 4He and the two "recycled" protons: 91% ...
the star
the star

... period of about one million years. Proxima Centauri is 4.22 light years from the Earth (now) and about 0.24 light years from Alpha-Centauri A and B. • Alpha-Centauri A and B – a double star system with a period of about 80 years. Component A is a near twin of the sun (Type G2). Component B is a lit ...
Spectra of Star Clusters
Spectra of Star Clusters

... stars in many phases of life, just as we might study how  humans age by observing the humans living in a village  at one time. • What two basic physical properties do astronomers use to  classify stars? • Stars are classified by their luminosity and surface  temperature. These properties, in turn, d ...
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Hipparcos



Hipparcos was a scientific satellite of the European Space Agency (ESA), launched in 1989 and operated until 1993. It was the first space experiment devoted to precision astrometry, the accurate measurement of the positions of celestial objects on the sky. This permitted the accurate determination of proper motions and parallaxes of stars, allowing a determination of their distance and tangential velocity. When combined with radial-velocity measurements from spectroscopy, this pinpointed all six quantities needed to determine the motion of stars. The resulting Hipparcos Catalogue, a high-precision catalogue of more than 118,200 stars, was published in 1997. The lower-precision Tycho Catalogue of more than a million stars was published at the same time, while the enhanced Tycho-2 Catalogue of 2.5 million stars was published in 2000. Hipparcos‍ '​ follow-up mission, Gaia, was launched in 2013.The word ""Hipparcos"" is an acronym for High precision parallax collecting satellite and also a reference to the ancient Greek astronomer Hipparchus of Nicaea, who is noted for applications of trigonometry to astronomy and his discovery of the precession of the equinoxes.
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