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Our Solar System I - hrsbstaff.ednet.ns.ca
Our Solar System I - hrsbstaff.ednet.ns.ca

... -Explain the theories for the origin of the solar system -Distinguish between questions that can be answered by science and those that cannot, and between problems that can be solved by technology and those that cannot with regards to solar system formation. -Estimate quantities of distances in pars ...
The Universe
The Universe

... distances in the Solar system; the Astronomical Unit, abbreviated as AU. One astronomical unit is the (average) distance from the Earth to the Sun; 149,597,870,700 metres, give or take a few metres. ...
Stars and Nebulae
Stars and Nebulae

... changes. The process of building up heavier elements from lighter ones by nuclear reactions, and adjusting the internal structure to balance gravity and pressure, is called stellar evolution. Looking at a star through a telescope can tell us many of its important properties. The color of a star tell ...
Stars
Stars

... In a star like the Sun, electron degeneracy stops the contraction of the core before the temperature gets high enough to start carbon burning. Supported against further contraction, the core cannot get any more energy by gravitational contraction. From this point on, the core cools down like an ordi ...
YSO/PMS disk types, time-scales and evolution from 1
YSO/PMS disk types, time-scales and evolution from 1

... statistics (Udry et al. 2007) suggest low are present after 10 Myrs ...
Sample Exam 1
Sample Exam 1

... 23. Saturn’s rings are clusters of relatively small, individual particles; the rings observed on Jupiter are violent storm clouds swirling above the polar regions of the planet. a. True b. False 24. Why do we see essentially the same face of the Moon at all times? a. because the Moon does not rotate ...
The human race has made great strides in the last few centuries
The human race has made great strides in the last few centuries

The colour-magnitude diagram
The colour-magnitude diagram

Mar 2017 - What`s Out Tonight?
Mar 2017 - What`s Out Tonight?

... everyone’s favorite because of its beautiful rings. Mars gets close galaxy like a halo. M22 in SAGITTARIUS is a northern favorite. to Earth about every 2 years at which time it is very bright. This A Planetary Nebula is an old term that has nothing to do is the best time to observe it but you need h ...
File - YEAR 11 EBSS PHYSICS DETAILED STUDIES
File - YEAR 11 EBSS PHYSICS DETAILED STUDIES

... extended the apparent magnitude scale upwards to 0 and then -1 and so on. The invention and development of telescopes allowed for the discovery of stars dimmer then +6, so the scale was extended downwards, +7 and so on. In the 19th century astronomers were able to more accurately quantify the appa ...
18th Cambridge Workshop on Cool Stars, Stellar Systems, and the... Proceedings of Lowell Observatory (9-13 June 2014)
18th Cambridge Workshop on Cool Stars, Stellar Systems, and the... Proceedings of Lowell Observatory (9-13 June 2014)

... session is the magnetism of planet-hosting stars (e.g., Fares et al., 2013, see also Section 6.). Interestingly, the only star other than the Sun for which a magnetic cycle has been directly observed with spectropolarimetry is τ Boo (Donati et al., 2008; Fares et al., 2009), which has a close-in pla ...
Presentation
Presentation

... surface temperature Small, cold stars stay for hundreds of billions of years Massive, hot stars will leave after a few million years ...
What is a T Tauri star?
What is a T Tauri star?

... Active (star/disk interactions, fast rotation) Sometimes releasing mass via polar outflows ...
Extrasolar Planetary Systems » American Scientist
Extrasolar Planetary Systems » American Scientist

On a New Primary Planet of our Solar System, Long Suspected
On a New Primary Planet of our Solar System, Long Suspected

... whether a mangled planet came from the wide space that is between Mars and Jupiter. Lambert was most likely conducted to the thoughts through the comparison of various distances of the planets from one another, and he must at that time have already found that the space from Mars to Jupiter is sudden ...
Lecture Nine (Powerpoint format) - Flash
Lecture Nine (Powerpoint format) - Flash

...  Manufactured lenses for Naval Observatory (where Pluto’s moon Charon was discovered) and the University of Chicago Yerkes Observatory (which just shut down research very recently).  In 1862, when testing a new 18 inch telescope at the Dearborn observatory at Northwestern University in Evanston, h ...
solar system form
solar system form

... much later by stars and are cast into space when stars die. By mass, 98% of the observed matter in the universe is hydrogen and helium. The solar system formed 4.6 billion years ago from a swirling, disk-shaped cloud of gas, ice, and dust, called the solar nebula. The four inner planets formed throu ...
“Crossroads of Astronomy.” Talk about Five Remarkable
“Crossroads of Astronomy.” Talk about Five Remarkable

... Henrietta also realized that "since the variables are probably nearly the same distance from the earth, their periods are apparently associated with their actual emission of light, as determined by their mass, density, and surface brightness." The Cepheids were in the Small Magellanic Cloud are all ...
Extreme Stars
Extreme Stars

... Mass: 0.8 Suns Sometimes fades by a factor of 1000 or more in brightness! Emits “puffs” of soot that block the light of the star ...
Unit 8 Chapter 30
Unit 8 Chapter 30

... The death takes millions of years, but when it gets to the core, it can take a few weeks to a few months. This becomes the source material for new stars/solar systems. ...
Birth of Elements
Birth of Elements

... discovered in the solar spectrum, produced by an element initially nicknamed "coronium", were finally identified with that of Helium which was discovered subsequently on the Earth. The picture below shows the spectrum of the sun with absorption lines2 (called Fraunhofer lines named after the German ...
Stars and the Main Sequence
Stars and the Main Sequence

... The origin of pressure: equation of state Under the simplest assumption of an ideal gas: ...
study guide
study guide

... • Some are large, most are captured asteroids ...
teachers` answers for Secondary Visit Guide and Activities
teachers` answers for Secondary Visit Guide and Activities

... Can you identify two ways he did this in his clocks (H1, H2, H3, H4) and learn more about them using the interactives? 1 Springs (This was unnecessary for the small movements in H4) 2 Bimetallic Strip. Harrison used this to curb the effect of temperature on the balance spring of H3. What other ...
Stars and Planets - The University of Texas at Dallas
Stars and Planets - The University of Texas at Dallas

... In the 1920’s Edwin Hubble not only showed that many “nebula” were in fact other galaxies, but that galaxies appear to be speeding away from one another. The further away a galaxy was (measured with standard candles), the faster it seemed to move away from us! velocity = Ho x distance, where Ho is a ...
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