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Navigation - hrsbstaff.ednet.ns.ca
Navigation - hrsbstaff.ednet.ns.ca

The Birth, Life, and Death of Stars
The Birth, Life, and Death of Stars

1” “Sky-Notes” of the Open University Astronomy Club. September
1” “Sky-Notes” of the Open University Astronomy Club. September

... Opposition was reached on 1st September. At magnitude +5.7 (diameter of nearly 4”) it is easily located in binoculars using a suitable star chart. ...
Binary star formation
Binary star formation

... • If Etotal < 0: stars are bound (don’t need to form a binary - we have one already!) • If Etotal > 0: stars are unbound and will remain so For one star to capture another and form a binary, need to somehow lose energy from the system. - into internal energy / fluid motion of the stars - give energy ...
The Constellations
The Constellations

astronomy practice Answers - hhs-snc1d
astronomy practice Answers - hhs-snc1d

... Practice Astronomy Questions Answers 1) If something were to happen to the sun, it would take __________ for us to know about it. a) 8 seconds b) 8 minutes c) 8 hours d) 8 days ...
April - Bristol Astronomical Society
April - Bristol Astronomical Society

... Due to the school holidays the first 2 meetings in April will be maintenance sessions at the observatory. there is always quite a lot of work to do in the spring as very little in the way of maintenance is carried out over the winter months. One of the main tasks is to shift all of the dead hedges t ...
8Sept103_2014
8Sept103_2014

... • Hypotheses that pass rigorous testing become Laws (more mathematical) or Theories (described using both words and equations). ...
s*t*a*r chart - Ontario Science Centre
s*t*a*r chart - Ontario Science Centre

Lecture 22 - Cosmic distance scale
Lecture 22 - Cosmic distance scale

Celestial Motions
Celestial Motions

... Earth determines which constellations remain below the horizon. (They depend on time of year because Earth’s orbit changes the apparent location of the Sun among the stars.) ...
Astronomical distances and Stellar magnitudes
Astronomical distances and Stellar magnitudes

... Astronomical distances and stellar magnitudes 1. What is meant by a light year? 2. What is meant by an astronomical unit (AU)? 3. What is meant by a parsec (pc)? 4. What is meant by a mega parsec (Mpc)? 5. What is meant by the apparent magnitude of an astronomical object? 6. Give the approximate dis ...
Document
Document

... • When a star is approaching the Earth, the light waves will be compressed. • The wavelengths are shorter and are characteristic of blue and violet light. • If the star is moving away from Earth, the waves will be expanded. Longer wavelengths are characteristic of red light. • The spectrum of a star ...
4P38.pdf
4P38.pdf

What is a star?
What is a star?

... • The sun is a star and is composed mostly of hydrogen and helium. It also contains oxygen, carbon, neon, and iron. • At the center of the sun lies the core, where gases are compressed and heated and temperatures reach 15 million degrees Celsius. • The sun’s core is where matter is converted into ...
Astronomy_Syllabus
Astronomy_Syllabus

... important, as it dealt with the question of the relationship between the Earth and all the heavenly bodies, including the Sun and Moon. Ancient cultures used their knowledge of the heavenly movements to regulate agricultural cycles, establish calendars, predict eclipses, and perform religious ritual ...
Specific Word Instruction Possible Sentences
Specific Word Instruction Possible Sentences

... stronomy is the study of the planets, stars, and galaxies. People have been watching the movement of the sun, moon, planets, and stars since ancient times. So astronomy is a very, very old science. From early times, people tried to make models of the universe. For many years, no one wanted to believ ...
The professional project VEGA/CHARA and participation of ASPA
The professional project VEGA/CHARA and participation of ASPA

absolute magnitude
absolute magnitude

... – If a star is actually closer than 10pc, its absolute magnitude will be a bigger number, i.e. it is intrinsically dimmer than it appears – If a star is farther than 10pc, its absolute magnitude will be a smaller number, i.e. it is intrinsically brighter than it appears ...
ph507lecnote06
ph507lecnote06

... Therefore, specialized techniques that can measure radial velocity shifts of ~10-3 of a pixel stably over many years are required High sensitivity to small radial velocity shifts is achieved by: • comparing high S/N = 200 - 500 spectra with template stellar spectra • using a large number of lines in ...
test - Scioly.org
test - Scioly.org

... B) as a main 5squsnse star. C) as a planetary nebula. D) as a red giant or supergiant. E) as a T Tauri variable star. 14) Higher mass protostars enter the main seque.lrce: A) faster and at a higher luminosity and temperature. B) faster and at a lower luminosity and temperature. C) slower and at a hi ...
Science: Astronomy Distance and Parallax
Science: Astronomy Distance and Parallax

... other words, Proxima has the same angular motion in Earth's sky that Earth has in Proxima's. This angular displacement, 1.546 arc seconds, corresponds to a distance of 266,757 astronomical units. Astronomers define parallax angle as one half of this angular displacement (in this case, 0.773 arc seco ...
Distance Measures: Parallax
Distance Measures: Parallax

Introduction to the sky
Introduction to the sky

Introduction to the sky
Introduction to the sky

... equator. It is a projection of the Earth's equator out to the celestial sphere. The number of degrees that a celestial object is north or south of the celestial equator is called the declination (DEC) It is the analogue of latitude on the sky. The analogue of longitude is called right ascension (RA) ...
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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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