• 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
Milankovitch Cycles and Glaciation
Milankovitch Cycles and Glaciation

... Variations in the Earth's eccentricity, axial tilt, and precession comprise the three dominant cycles, collectively known as the Milankovitch Cycles for Milutin Milankovitch, the Serbian astronomer who is generally credited with calculating their magnitude. Taken in unison, variations in these three ...
Astrophysics
Astrophysics

... Sunspots are the most dominant features on the Sun surface. They harbour complex concentrations of magnetic field that become entangled in the plasma ocean that is solar surface, otherwise known as the photosphere. They migrate across the solar disk, close to the solar equator, and they can rapidly ...
–1– AST104 Sp2006: EXAM 1 Multiple Choice Questions: Mark the
–1– AST104 Sp2006: EXAM 1 Multiple Choice Questions: Mark the

... e. 105 times brighter than what angle would you measure between the north13. The 26,000 year precession cycle of the Earth’s ern horizon and the Zenith? spin axis implies that a. 62 degrees a. Polaris will not always be the star currently nearest to the North Celestial Pole. b. 5 degrees c. 90 degre ...
PowerPoint
PowerPoint

... 1. The extent of the moon in the sky is about 30 arcminutes. 2. The moon is big 3. The moon takes about 60 arcseconds to rise. 4. The extent of the moon in the sky is about 30 arcseconds. 5. The moon takes about 60 arcminutes to rise. ...
Comets - Cloudfront.net
Comets - Cloudfront.net

... Comets are spectacular celestial objects. They appear suddenly are there for a few weeks or months And then disappear. Until the 1700’s Comets were thought to be unique events, often believed to be omens of disaster….such as the death of Kings For example the Normans used the appearance of a comet t ...
lecture9 Solar System1
lecture9 Solar System1

... Kuiper Belt object can be redirected by Neptune, creating a shortperiod comet. ...
AST 301—Review for Exam 3 Consult “Guide to Reading and Study
AST 301—Review for Exam 3 Consult “Guide to Reading and Study

... that there are several techniques that could be used to detect extrasolar planets, but that basically only one has been so far successful (with a few recent detections using another technique). Can you explain why that is? (We also went over this in class.) Of the numerous extrasolar planets that ha ...
Earth-Moon-Sun System (seasons, moon phases
Earth-Moon-Sun System (seasons, moon phases

... During the northern hemisphere’s summer (when the axis points towards the Sun), it receives sunlight for a longer time (longer days, shorter nights) as well as more directly. (The Sun is higher in the sky, so it hits the surface more directly.) Moving from the equator to the poles, the length of th ...
The Solar System 2015
The Solar System 2015

... Apart from the eight planets in the Solar System, there is also known a few hundreds of extrasolar planets, which orbit foreign stars. Contemporary astronomical instruments do not allow to observe these distant planets directly, but their properties are calculated from photometric and astrometric m ...
Course Expectations
Course Expectations

... Astronomy Course Expectations Unit 1 Exploring the Sky Understand 1. Scientific explanations change over time when new evidence conflicts with the existing theory. 2. Technological advances enable science to collect new evidence to support or disprove theories. 3. Matter emits or absorbs electromagn ...
8th Grade 2nd Semester Test Chapters 13, 16, 18
8th Grade 2nd Semester Test Chapters 13, 16, 18

... b. Regions with many craters c. Regions formed from huge lava flows d. Lunar highlands 48. The goal of the Apollo program was to a. Land astronauts on the moon b. Established a permanent colony on the moon c. Put the first American in space d. Prove that the moon is solid 49. The main advantage of a ...
Study of the movement of the sun through the analysis of a shade.
Study of the movement of the sun through the analysis of a shade.

... Second week in April Preparation and execution of the second measurement day. o In the second day of measurements, all the students within 1ºESO were invited to join. The aim of the project as well as the results of the two measurements were presented and explained to the new students. Due to the pl ...
The Moon - Kaufman ISD
The Moon - Kaufman ISD

... weigh more on the Earth than on the moon? ...
A WALK THROUGH THE SOLAR SYSTEM
A WALK THROUGH THE SOLAR SYSTEM

... Ancient astronomers observed points of light that appeared to move among the stars, and they called these objects planets, meaning wanderers. They were named after Roman legends. Jupiter was the king of the gods, Mars the god of war, Mercury was messenger of the gods, Venus was the god of beauty, an ...
Venus Transit Info on Measuring Distances
Venus Transit Info on Measuring Distances

... just means that Venus will be between the Earth and Sun, so that Venus will appear as a small dot on the Sun’s surface. Scientists studied the Venus transits in the eighteenth century in order to calculate the distance to the Sun, and to the other planets in our solar system. This was one of the mos ...
ph507-16-6sun
ph507-16-6sun

... The number of sunspots (R=f+10*g) on the Sun varies on an 11-year cycle. The number increases from zero at solar minimum, to over 100 at solar maximum, 5 1/2 years later. Every 11 years the polarity of the Sun's magnetic field flips. Therefore, the Sun's magnetic field varies on a 22-year cycle. As ...
Stars
Stars

... As a star collapses in a supernova its magnetic field is prevserved, but intensified as it is squeezed into a smaller object. Similarly the neutron star will rotate, as did the original star, but much faster (think about a twirling ice skater). Charged particles trapped by the magnetic field will ra ...
Final Exam from 2004 - Onondaga Community College
Final Exam from 2004 - Onondaga Community College

... timescales and angles and the difference in the apparent motion between the summer Sun and the winter Sun. (7 pts) 2. Imagine you have been invited to attend a graduation party for the daughter of the President of the company you are working for. The daughter has just received her B.S. in Physics. Y ...
The Sun: A Model Star
The Sun: A Model Star

... The number of sunspots (R=f+10*g) on the Sun varies on an 11-year cycle. The number increases from zero at solar minimum, to over 100 at solar maximum, 5 1/2 years later. Every 11 years the polarity of the Sun's magnetic field flips. Therefore, the Sun's magnetic field varies on a 22-year cycle. As ...
Pre SS1 Models of the Solar System - Bolinas
Pre SS1 Models of the Solar System - Bolinas

... the apparent brightness of stars along the zodiac; in summer, for instance, when the Earth is on the side of its orbit closer to the star Spica, its proximity would make Spica look brighter than it does in winter, when the Earth is on the far side of its orbit. As no such phenomenon is observed, the ...
ppt
ppt

... The remaining planetesimals close to the Sun will almost all impact with planets in this region ...
SWFAS Sept 2016 Newsletter - Southwest Florida Astronomical
SWFAS Sept 2016 Newsletter - Southwest Florida Astronomical

... was able to raise $25,730 towards the construction of a state-of-the-art observatory. Bond designed the building and the observing chair (both of which are still in working order today), and Harvard bought a fifteen-inch German-built refracting telescope, equal in size to the largest in the world at ...
TTh HW02 key
TTh HW02 key

... How much of the total surface of the Moon is illuminated by the Sun when it is at quarter phase? one quarter very little all of it one half ...
Lecture 6 Recall: Geocentric Model of Solar System
Lecture 6 Recall: Geocentric Model of Solar System

... exactly uniform motion in circles around the Sun, which still did not agree that well with the observations. – This problem was fixed by Kepler, who removed the assumption of uniform motion in circles (see below) • Heliocentric model has multiple centers: Moon goes around Earth, Earth and other plan ...
Gravitation
Gravitation

... The largest known asteroid in the solar system is Ceres, which is located in an orbit between Mars and Jupiter. Although the existence of Ceres has been known for two hundred years, its mass is still not well determined. Suppose the magnitude of the gravitational force between the sun and Ceres equa ...
< 1 ... 108 109 110 111 112 113 114 115 116 ... 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