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Glossary - Royal Astronomical Society of Canada
Glossary - Royal Astronomical Society of Canada

... indistinct, non-terrestrial objects visible in the night sky; “bright” nebulae glow with light emitted by the gas of which they are composed (“emission” nebulae) or by starlight reflected from dust (“reflection” nebulae) or both; “dark” nebulae consist of clouds of gas and dust that are not so illum ...
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exam_1fall_01

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Astronomy 10: Introduction to General Astronomy Instructor: Tony
Astronomy 10: Introduction to General Astronomy Instructor: Tony

... When we measure velocities of stars using Doppler shifts, it can only measure the radial velocity (that is, the velocity directly toward or away form us). In general, the orbit can be at an angle from us, so that the true orbital velocity is equal or greater than what we measure. In turn the inferre ...
angular size - Particle and Astroparticle Physics
angular size - Particle and Astroparticle Physics

... • The basic unit of angular measure is the degree (°). • Astronomers use angular measure to describe the apparent size of a celestial object—what fraction of the sky that object seems to cover • The angular diameter (or angular size) of the Moon is ½° or the Moon subtends an angle of ½°. ...
sunmoon - University of Glasgow
sunmoon - University of Glasgow

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Clever Catch - American Educational Products
Clever Catch - American Educational Products

... The Sun, planets, comets, and moons are all part of our _______ . ...
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IMPORTANT HISTORICAL DATES AND EVENTS

... As it formed from the gas and grit of the solar nebulae, the sun sucked in virtually all matter for billions of miles, ending up with more than 98.8% of the solar system’s mass. Nuclear fusion in its core powers the sun. The enormous heat and pressure generated within the sun’s centre, fusing hydrog ...
powerpoint - High Energy Physics at Wayne State
powerpoint - High Energy Physics at Wayne State

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Origin of Modern Astronomy
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Chapter 11
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PowerPoint Presentation - AY 4: The Stars

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... capable of surviving at extreme climates, and a sun with double the temperature and 16 times the power would certainly produce extreme climates. At those temperatures, it's likely that the polar ice caps would melt and cause extreme flooding. Additionally, with the sun's peak wavelength dropping by ...
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Chapter 5 - AstroStop

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Glossary of terms - Universal Workshop
Glossary of terms - Universal Workshop

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Our Star, the Sun - Solar Physics and Space Weather
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... members”, while the sunspots following behind are called “following members” • In one solar hemisphere, the preceding members all have the same magnetic polarity; the following members have the opposite polarity • The polarity is opposite in the other hemisphere ...
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07-TysonsZodiacAreTh.. - Saptarishis Astrology

... Scorpius, the sign that is advertised to precede Sagittarius. The confusing conclusion is that most Scorpions are actually Ophiuchans, and all Scorpions and Ophiuchans are currently Librans. The fourteenth constellation in the set is Cetus. It is a large constellation that dips into Pisces. The Sun ...
The Ever-Changing Sky
The Ever-Changing Sky

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Section 7.3 - CPO Science
Section 7.3 - CPO Science

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The Sun
The Sun

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< 1 ... 118 119 120 121 122 123 124 125 126 ... 228 >

Tropical year

A tropical year (also known as a solar year), for general purposes, is the time that the Sun takes to return to the same position in the cycle of seasons, as seen from Earth; for example, the time from vernal equinox to vernal equinox, or from summer solstice to summer solstice. Because of the precession of the equinoxes, the seasonal cycle does not remain exactly synchronized with the position of the Earth in its orbit around the Sun. As a consequence, the tropical year is about 20 minutes shorter than the time it takes Earth to complete one full orbit around the Sun as measured with respect to the fixed stars (the sidereal year).Since antiquity, astronomers have progressively refined the definition of the tropical year. The Astronomical Almanac Online Glossary 2015 states:year, tropical:the period of time for the ecliptic longitude of the Sun to increase 360 degrees. Since the Sun's ecliptic longitude is measured with respect to the equinox, the tropical year comprises a complete cycle of seasons, and its length is approximated in the long term by the civil (Gregorian) calendar. The mean tropical year is approximately 365 days, 5 hours, 48 minutes, 45 seconds.An equivalent, more descriptive, definition is ""The natural basis for computing passing tropical years is the mean longitude of the Sun reckoned from the precessionally moving equinox (the dynamical equinox or equinox of date). Whenever the longitude reaches a multiple of 360 degrees the mean Sun crosses the vernal equinox and a new tropical year begins"". (Borkowski 1991, p. 122)The mean tropical year on January 1, 2000, was about 365.2421897 ephemeris days according to the calculation of Laskar (1986); each ephemeris day lasting 86,400 SI seconds. By 2010 this had decreased to 365.2421891 (365 ephemeris days, 5 hours, 48 minutes and 45.14 seconds). This is about 365.242181 mean solar days, though the length of a mean solar day is constantly changing.
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