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Stellar Nucleosynthesis
Stellar Nucleosynthesis

A105 –Stars and Galaxies
A105 –Stars and Galaxies

... Estimate the period of the orbit (the time for one complete orbit, or the time between maximums (or minimums) in the velocity curve). What is the length of the “year” of 51 Peg’s planet? Next, estimate the mass of 51 Peg’s planet. The following graph relates the mass of the planet to the range of ve ...
Measuring Stars
Measuring Stars

... In many cases a binary system is too far away, or the stars are too close, or one star is so much brighter than the other that we cannot distinguish the two stars visually. But still we can infer that the system is binary by several indirect methods. – Eclipsing binaries: In some binary systems orbi ...
Slide 1
Slide 1

... 8) Which of the following statements is NOT true: a) A reindeer grows a new set of antlers every year b) Reindeers have a poisonous spine on their back legs c) The reindeer is the only species where the males AND females grow antlers d) A reindeer’s antlers can grow up to 1.3m long ...
The Electromagnetic Spectrum: Astronomy 1
The Electromagnetic Spectrum: Astronomy 1

Document
Document

... Orion Nebula. Can you spot the star Betelgeuse, which shows up as a blue/white dot in the upper centre? The ring to the right of Betelgeuse is the remnant of a supernova (the dying explosion of a giant star). ...
HEIC0410: FOR RELEASE 15:00 (CEST)/9:00 AM EDT 15 June
HEIC0410: FOR RELEASE 15:00 (CEST)/9:00 AM EDT 15 June

... Both components of the binary system belong to the L spectral class that includes the lowest mass stars and the highest mass brown dwarfs in our solar neighbourhood. This spectral class was discovered in 1997 and was added to the spectral classification that had remained unchanged for half a century ...
here - British Astronomical Association
here - British Astronomical Association

Stellar Evolution
Stellar Evolution

... Observing Stellar Evolution in Star Clusters The following series of H-R diagrams shows how stars of the same age, but different masses, appear as the whole cluster ages. After 10 million years, the most massive stars have already left the Main Sequence, while many of the least massive have not eve ...
Astronomy - Scioly.org
Astronomy - Scioly.org

... e. They are fully connective, and never develop a hydrogen shell fusion zone. 53. What type of spectrum does the gas in a planetary nebula produce? a. A continuous spectrum. b. An emission line spectrum. c. An absorption line spectrum. d. An emission line spectrum superimposed on a continuous spectr ...
Extension worksheet – Topic 6 - Cambridge Resources for the IB
Extension worksheet – Topic 6 - Cambridge Resources for the IB

... 4 b to measure distance and Spectroscopic parallax makes use of the formula so requires knowledge of luminosity and apparent brightness; apparent brightness can easily be measured with a CCD camera; the luminosity can be determined if we know the temperature of the star (obtained form its spectrum) ...
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Source: https://www

not - ISDC
not - ISDC

... ● Let’s start with some astronomy... ...
Chapter 16 - "The Universe"
Chapter 16 - "The Universe"

... use a two-coordinate horizon system to locate positions in the sky. – One popular method of using this system identifies the altitude angle (in degrees) from the horizon up to an object on the celestial sphere and the azimuth angle (again in degrees) the object on the celestial sphere is east or wes ...
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hubble amazing universe worksheet

... 7. In 2005, the Corina nebula was revealed. The data comes back in ________________ and ____________________, and gasses are assigned colors. Blue is ___________, and green is ___________________. 8. This region is _____________ light years across! 9. Hubble even showed a star about to die! As a sta ...
Events: - Temecula Valley Astronomers
Events: - Temecula Valley Astronomers

... As the sun sets, I try to point out the first stars visible - usually the summer triangle. I talk about constellations and asterisms. Once the sky is dark, our first targets are man-made satellites. Many web sites and cell phone apps help you find what is visible. While we are waiting for them to co ...
Constellations
Constellations

$doc.title

... Use  Star  Walk  or  your  team’s  own  naked-­‐eye  observations  to  check  the  accuracy  of  your  finding  chart.  If  your   chart  does  not  correctly  show  the  position  of  the  planet,  explain  what  went  wrong:     ...
34ReviewNuclear
34ReviewNuclear

Spectrum a Star….. - SFA Physics and Astronomy
Spectrum a Star….. - SFA Physics and Astronomy

... Mystery Star Properties 1. The star appears as a point of light through a telescope. 2. The absorption lines appear split and move over a 4 day period. 3. The brightness of the star also varies over 4 days. Question: Why do you think the brightness of the star is varying? Answer: This could be an e ...
LIGHT VS. DISTANCE
LIGHT VS. DISTANCE

... The “Gamma ray” song We know that gamma ray explosions happen randomly all over the sky (It's like a lottery: a ticket for each square degree) You see a FLASH! and then there's not another till about a day ...
Messier Galaxies of #202541
Messier Galaxies of #202541

Constellations
Constellations

... Rising and Setting Stars • Other stars “move” in circles about Polaris. • It takes 1 day to complete the circle. • The rising and setting time of a star changes with the ...
Stars & Constellations
Stars & Constellations

... Navigation utilises constellations - it helps locate a specific star, such as Polaris (the North Star). Knowing this, plus how high the star is in the sky gives a navigator their direction + their latitude (how far North / South they are) ...
Jeopardy 2015
Jeopardy 2015

... 100 billion stars The Milky Way Contains which of the following: 100,000 stars 100 million stars 100 Billion stars ...
< 1 ... 156 157 158 159 160 161 162 163 164 ... 262 >

Lyra



Lyra (/ˈlaɪərə/; Latin for lyre, from Greek λύρα) is a small constellation. It is one of 48 listed by the 2nd century astronomer Ptolemy, and is one of the 88 constellations recognized by the International Astronomical Union. Lyra was often represented on star maps as a vulture or an eagle carrying a lyre, and hence sometimes referred to as Aquila Cadens or Vultur Cadens. Beginning at the north, Lyra is bordered by Draco, Hercules, Vulpecula, and Cygnus. Lyra is visible from the northern hemisphere from spring through autumn, and nearly overhead, in temperate latitudes, during the summer months. From the southern hemisphere, it is visible low in the northern sky during the winter months.The lucida or brightest star—and one of the brightest stars in the sky—is the white main sequence star Vega, a corner of the Summer Triangle. Beta Lyrae is the prototype of a class of stars known as Beta Lyrae variables, binary stars so close to each other that they become egg-shaped and material flows from one to the other. Epsilon Lyrae, known informally as the Double Double, is a complex multiple star system. Lyra also hosts the Ring Nebula, the second-discovered and best-known planetary nebula.
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