• Study Resource
  • Explore Categories
    • Arts & Humanities
    • Business
    • Engineering & Technology
    • Foreign Language
    • History
    • Math
    • Science
    • Social Science

    Top subcategories

    • Advanced Math
    • Algebra
    • Basic Math
    • Calculus
    • Geometry
    • Linear Algebra
    • Pre-Algebra
    • Pre-Calculus
    • Statistics And Probability
    • Trigonometry
    • other →

    Top subcategories

    • Astronomy
    • Astrophysics
    • Biology
    • Chemistry
    • Earth Science
    • Environmental Science
    • Health Science
    • Physics
    • other →

    Top subcategories

    • Anthropology
    • Law
    • Political Science
    • Psychology
    • Sociology
    • other →

    Top subcategories

    • Accounting
    • Economics
    • Finance
    • Management
    • other →

    Top subcategories

    • Aerospace Engineering
    • Bioengineering
    • Chemical Engineering
    • Civil Engineering
    • Computer Science
    • Electrical Engineering
    • Industrial Engineering
    • Mechanical Engineering
    • Web Design
    • other →

    Top subcategories

    • Architecture
    • Communications
    • English
    • Gender Studies
    • Music
    • Performing Arts
    • Philosophy
    • Religious Studies
    • Writing
    • other →

    Top subcategories

    • Ancient History
    • European History
    • US History
    • World History
    • other →

    Top subcategories

    • Croatian
    • Czech
    • Finnish
    • Greek
    • Hindi
    • Japanese
    • Korean
    • Persian
    • Swedish
    • Turkish
    • other →
 
Profile Documents Logout
Upload
Eratosthenes Determines the Size of the Earth in about 200 B.C.
Eratosthenes Determines the Size of the Earth in about 200 B.C.

... “ecliptic”, which is tilted 23.5° with respect to the celestial equator. •  It appears to us that the Sun travels around the Celestial Sphere once a year. A parallax effect: as we orbit Sun, it is projected against different stars. After 1 year, it returns to same position relative to the stars (ecl ...
Earth has formed in our solar system
Earth has formed in our solar system

... because of cooling • Hence location is important for planetary composition (planets closer to the sun should be more refractory) • Interaction of large body at final stages could change composition considerably ...
sky science study notes
sky science study notes

... ‘gnomon’. To work best, a sundial must be designed for a specific place on the planet and adjusted for the time of year. ...
How Big Is Big
How Big Is Big

... 14. How Big Is REALLY Big? Every dot of light in the picture is a ____________. 15. Galaxies are collections of hundreds of _________ of stars. A galaxy is ________ times larger than the largest star. Many if not most stars have their own planets – called ____________. In every direction you can poi ...
Lab Activity on Variations in the Apparent Daily Path of
Lab Activity on Variations in the Apparent Daily Path of

... Earth inside the Celestial Sphere to spin. Notice that the stars do not move, only the Earth does (the moon and the other planets would too--if they were incorporated into this model). 2. In order to model the sky as seen from Chico, tilt and rotate the model celestial sphere until Chico is at the “ ...
One way to measure distance
One way to measure distance

... index finger at me. Close one eye then open the other. What happens? ...
Name - MIT
Name - MIT

... A) the universe will stop expanding and start contracting B) the universe will continue expanding C) the universe will start forming more supernovas D) the universe will start forming more stars E) the universe will start becoming warmer 11) The force that binds protons together in the nucleus is ca ...
Presentation
Presentation

... model that allowed prediction of planetary positions. • What are Kepler’s three laws of planetary motion? • (1) The orbit of each planet is an ellipse with the Sun at one focus. (2) As a planet moves around its orbit, it sweeps out equal areas in equal times. (3) More distant planets orbit the Sun a ...
Tennessee Academic Vocabulary Word Calendar
Tennessee Academic Vocabulary Word Calendar

... Raineshaven Elementary’s ...
The Sun and the Stars
The Sun and the Stars

... so far away from the Earth. This distance is measured in light-years, not in miles or kilometers. (One light-year is equal to the distance that light travels in one year. This is about six trillion miles or ten trillion kilometers!) Stars look like they are twinkling because when we see them, we are ...
IQ 2
IQ 2

... IQ • True! The Earth’s rotation causes the entire sky to appear to sweep from east to west once each day. • This is (generally) the “fastest” motion we notice. • The Earth’s rotation axis points at the north and south poles of the “celestial sphere.” • The Earth’s equator projects to the equator of ...
Sample pages 2 PDF
Sample pages 2 PDF

... • Zenith, Nadir: the points above and below the observer. • Meridian: the great circle that intercepts the poles, the zenith, and the nadir. The celestial objects show an apparent motion in the sky, rising, achieving a maximum altitude above the horizon, and setting. The objects can be observable du ...
Solar System where_are_we
Solar System where_are_we

... Galaxy Because we dwell within the Milky Way Galaxy, it is impossible for us to take a picture of its spiral structure from the outside. But we do know that our Milky Way has a spiral nature from observations made from within our Galaxy (though whether or not it is a barred spiral is still being deb ...
Quiz Questions
Quiz Questions

... D. heat from gravitational contraction 4. Why does hydrogen fusion only occur in the deep interiors of the Sun (and other stars)? A. because this is the only place in the Sun where there is sufficient hydrogen B. because only in the core is the temperature low enough and the density high enough C. b ...
Glossary - Sky Science
Glossary - Sky Science

... in the upper atmosphere above the poles. ...
astronomy ch 2 - Fort Thomas Independent Schools
astronomy ch 2 - Fort Thomas Independent Schools

... How much force does it take to keep an object moving in a straight line at a constant speed? Unless an object is subject to an outside force, it takes no force at all to keep it moving in a straight line at a constant speed. How does an object’s mass differ when measured on the Earth and on the Moon ...
Our Solar System
Our Solar System

... Our Solar System • Jupiter (5th planet from the Sun) – Largest planet in our solar system. – Its outer layer are made up of swirling gases. – Jupiter’s atmosphere is very colorful and it has an are called the Great Red Spot. • This spot is a storm that has been raging from hundreds of years and is ...
Lecture 13. Black Holes - Politechnika Wrocławska
Lecture 13. Black Holes - Politechnika Wrocławska

... • This is what we call a black hole. • The star becomes very small. – it creates a “hole” in the Universe – That not even light could escape ...
Navigating by the Stars
Navigating by the Stars

... This is now called Kepler's First Law or The Law of Ellipses. What is an ellipse? Glad you asked. An ellipse is a closed, curved shape that is defined by two foci. An ellipse is a like a flattened circle. In fact, if both of the foci of an ellipse are at the same point, an ellipse becomes a circle! ...
lecture5 - UMass Astronomy
lecture5 - UMass Astronomy

... Earth. You can now imagine how Earth, the moon, and the sun move through space and how that produces the sights you see in the sky. But how did humanity first realize that we live on a planet moving through space? That required revolutionary overthrow of an ancient and honored theory of Earth’s plac ...
Lecture 7: The Sun - Department of Physics and Astronomy
Lecture 7: The Sun - Department of Physics and Astronomy

... They can be tested, and disproven, but they can’t be tested in every in instance. A theory cannot be proven like a mathematical theorem. A theory may turn out to be a useful approximation, example: Newton’s laws are an approximation: they are superseded by Einstein’s theory of relativity on large ...
Stars: Element factories.
Stars: Element factories.

... more atoms having the same atomic number but different mass numbers. ...
Grade 7 Science
Grade 7 Science

... Constellations in the sky. The 12 constellations make up a ―belt‖ in the sky called the zodiac. Each month, the sun appears to be in a different constellation. The ancient Babylonians developed a 12month calendar based on the idea that the sun moved through this circle of constellations as it revolv ...
Chapter 08
Chapter 08

... is highly opaque to radiation. But neutrinos can penetrate huge amounts of material without being absorbed. Early solar neutrino experiments detected a much lower flux of neutrinos than expected (the “solar neutrino problem”). Recent results have proven that neutrinos change (“oscillate”) between di ...
Astro-Spectroscpy
Astro-Spectroscpy

... stellar atmosphere (not shown) ...
< 1 ... 132 133 134 135 136 137 138 139 140 ... 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.
  • studyres.com © 2025
  • DMCA
  • Privacy
  • Terms
  • Report