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Profile Documents Logout
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Sections F and G
Sections F and G

... We can image different layers of the Sun using radiation at different wavelengths since these are emitted or absorbed differently. Recall from Astrophysical Concepts, the idea of ‘optical depth’. If radiation of intensity I0 is incident on one side of a slab of material of thickness x then the emerg ...
Earth Science 25.2A : Stellar Evolution
Earth Science 25.2A : Stellar Evolution

... life spans.  These stars end in a brilliant explosion called a supernova.  During a supernova, a star becomes millions of times brighter than it’s prenova stage.  If one of the stars nearest to Earth produced a supernova, it would be brighter than our sun. ...
Lecture 17 Review
Lecture 17 Review

... star is too large, the gas cloud condenses quite fast, is unstable, gets very hot, and either explodes or fragments into smaller clouds which form individual stars. A second question is, can the mass of the gas be too small. The answer is yes. If the mass of the cloud is too small it heats up from g ...
Dark blue dot not so dark
Dark blue dot not so dark

... “This can happen if there is enough gas in the cloud core to provide resistance,” said the paper’s lead author, Bo Reipurth of the Institute for Astronomy at the University of Hawaii at Manoa. “Sometimes there is so much gas in the core that the two close stars spiral all the way in and collide with ...
Transcript of lecture I
Transcript of lecture I

Document
Document

... with a telescope. Spectroscopic observations show periodic Doppler shifts in the spectra of Mizar A and B, indicating that they are each binary stars. But they were too close to be directly imaged - until 2 May 1996, when the NPOI produced the first image of Mizar A. That image was the highest angul ...
Lab #5 (Feb 27
Lab #5 (Feb 27

... Within this exercise, select Part 1: The Moon’s Rotation. This exercise will ask you to determine the length of a sidereal day on the Moon, and we will also determine the length of a solar day. Just as a sidereal day is the amount of time it takes for a star to return to the meridian, the solar day ...
Stars
Stars

... with a telescope. Spectroscopic observations show periodic Doppler shifts in the spectra of Mizar A and B, indicating that they are each binary stars. But they were too close to be directly imaged - until 2 May 1996, when the NPOI produced the first image of Mizar A. That image was the highest angul ...
Nebular theory
Nebular theory

... Our theory about how the solar system formed is called the nebular theory. This activity will help you understand how we think the solar system formed. 1. Write your observations from the video that shows how the planets orbit the sun. Write at least 4 observations. Look for similarities, difference ...
Astronomy – The Milky Way Galaxy
Astronomy – The Milky Way Galaxy

... Large Magellanic Cloud and Small Magellanic Cloud orbit the Milky Way at 150,000 light years and 200,000 light years. ...
Key Notes for Test 1
Key Notes for Test 1

... This gives IR out per unit area as 345 (watts m-2 ), then we use the Stefan-Boltzmann Law , E (Joules m-2 s-1 ) = Teq4 , to work out the temperature. This tells us that the Temperature at equilibrium, Teq, must be Teq = (E/)¼ Using the full Solar Constant this gives an expected equilibrium tempera ...
Measuring the Stars
Measuring the Stars

... the period and semi-major axis of the orbit must be measured. •Kepler’s third law gives the sum of the masses of the two stars. •Relative speeds of the two stars can be measured using the Doppler effect •Speed will be inversely proportional to the mass. This allows us to calculate the mass of each s ...
Introduction: Gravity
Introduction: Gravity

... Earth’s daily spin in relation to the sun caused day and night. (4-5 ES1B) The moon has predictable phases that change how we view the moon from the Earth. (1-2 ES1C) Earth’s nearly circular yearly orbit around the sun causes us to see different constellations at different times of the year. (4-5 ES ...
see figure - Georgia Southwestern State University
see figure - Georgia Southwestern State University

... The total phase may last just a few seconds, or it may last as long as about 7 minutes. (The next eclipse to be almost that long will cross China near Shanghai on July 22, 2009, though the maximum duration will be available only over the Pacific ocean, and people on land will have to settle for “onl ...
The difference between asteroids and meteorites
The difference between asteroids and meteorites

... Asteroids are sometimes referred to as minor planets or planetoids, but in general, they are rocky bodies that do not have an atmosphere. However, a few have their own moons. Our solar system contains millions of asteroids, many of which are thought to be the shattered remnants of planetesimals – bo ...
Student Text, pp. 139-144
Student Text, pp. 139-144

... of the universe. Astronomers studied the motion of Uranus over many years and discovered that its path was not quite as smooth as expected. Some distant hidden object appeared to be “tugging” on Uranus causing a slightly uneven orbit. Using detailed mathematical analysis, they predicted where this h ...
Gresham Lecture, Wednesday 15 December 2010 Unsolved
Gresham Lecture, Wednesday 15 December 2010 Unsolved

Complete the following review packet!
Complete the following review packet!

PPT
PPT

... • The overall range of stellar masses runs from 0.08 times the mass of the Sun to about 150 times the mass of the Sun. • Masses are only known for stars that form binary systems, but about half of all stars are in fact in binary systems! – 0.08 MSun is approximately 80 MJupiter ...
Cairo Governorate Helwan Education Zone El
Cairo Governorate Helwan Education Zone El

... 1. The somatic cell contains ............... number of chromosomes while the gametes contains ............... number of chromosomes. 2. There are two kinds of mirrors which are ...............and ............... 3. The earth rotates around the ............... while the sun rotates around the center ...
Satellite stuff - Ms. Gamm
Satellite stuff - Ms. Gamm

Supernova Stalking - Susanna Kumlien Reportage
Supernova Stalking - Susanna Kumlien Reportage

... into perspective. Which is one of the many reasons as to why the sudden flare-up of supernovae on the dynamic starry sky is of such interest to Science. Not only are they spectacular events, but supernovae hold many secrets of great importance for our understanding of the universe, life and everythi ...
THE LIFE CYCLE OF STARS
THE LIFE CYCLE OF STARS

Volcanoes and Igneous Activity Earth
Volcanoes and Igneous Activity Earth

... • Stars with masses similar to the sun evolve in essentially the same way as low-mass stars. • During their collapse from red giants to white dwarfs, medium-mass stars are thought to cast off their bloated outer layer, creating an expanding round cloud of gas called planetary nebula. ...
Star and Galaxies
Star and Galaxies

... • Stars with masses similar to the sun evolve in essentially the same way as low-mass stars. • During their collapse from red giants to white dwarfs, medium-mass stars are thought to cast off their bloated outer layer, creating an expanding round cloud of gas called planetary nebula. ...
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Timeline of astronomy

Timeline of astronomy around 2300 BC.
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