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Angular Measurement
Angular Measurement

... The distance that light, moving at a constant speed of 300,000 km/s, travels in one year. One light year is about 10 trillion kilometers ...
formation of stars
formation of stars

... neutron stars, and black holes. ...
Definitions
Definitions

... from a given latitude on Earth, never disappears below the horizon, due to its proximity to one of the celestial poles. Visible for the entire night (and throughout the day if it wasn’t for the sun’s glare) every night of the year. ...
1 Name: Date: PARALLAX EXERCISE1 The goal of this
1 Name: Date: PARALLAX EXERCISE1 The goal of this

... Compare the Sun to another star in the sky. They look completely different, and it was once believed that they were different types of objects. In fact, the Sun was once considered a planet! We now know the Sun is just another star, and the reason that the Sun appears different to us is that it is s ...
Extragalactic AO Science
Extragalactic AO Science

... Lyman-break galaxies, sub-mm galaxies, and ultraluminous infrared galaxies. Allow studies of stellar populations as a controlled function of radius. Improves Strehl since extragalactic sources have depended on off-axis guide stars. Generally beneficial to all areas of extragalactic science. ...
Teacher Guide - Astronomy Outreach at UT Austin
Teacher Guide - Astronomy Outreach at UT Austin

... progresses, students develop an understanding of the most fundamental concepts in stellar astronomy. The most important ideas are repeated through out the play. At the conclusion of the activity, students will have an understanding of the main three types of stars (red, yellow, and blue stars) and t ...
n at ionalnewsletter - Royal Astronomical Society of Canada
n at ionalnewsletter - Royal Astronomical Society of Canada

... News has been released that Vancouver Museums and Planetarium will build an astronomical observatory through a donation from the Gordon T. Southam family and the Provincial Government. The observatory will be named the MacMillan Southam Observatory, and will be built in Vanier Park, near the Planeta ...
PHYSICS 1500 - ASTRONOMY TOTAL: 100 marks Section A Please
PHYSICS 1500 - ASTRONOMY TOTAL: 100 marks Section A Please

PPV_hd169142
PPV_hd169142

... registered PSF template star observations (spectral types A0-A8; J-H ± 0.3 of HD 169142A), non-instrumentally scattered circumstellar light is seen in all PSF subtracted images where the underlying PSF structure is well matched to the HD 169142A observations. Fig. 2: 2MASS 18242929-2946559 is reveal ...
Motion of stars, planets
Motion of stars, planets

... 1. The Copernican model has a force between the sun and the planets. Actually, the natural motion of the celestial spheres drove the planetary motions. 2. The Copernican model was simpler than the Ptolemaic one. In fact, though Copernicus eliminated circles to explain retrograde motion, he added mor ...
Feb 2017 - What`s Out Tonight?
Feb 2017 - What`s Out Tonight?

Conceptobasico.pdf
Conceptobasico.pdf

... farther away appear fainter); the wavelengths considered (some objects are brighter at infrared or ultraviolet wavelengths than in visible light); the sensitivity of the detector (the eye is less sensitive to blue light than standard photographic film). With absolute magnitude, one can compare the " ...
Tour the sky`s reddest stars
Tour the sky`s reddest stars

... © 2010 Kalmbach Publishing Co. This material may not be reproduced in any form without permission from the publisher. www.Astronomy.com ...
Stars and The Universe
Stars and The Universe

... Stellar Evolution: The Deaths of Stars a. A Second Red-Giant Phase ...
Circumpolar constellations
Circumpolar constellations

... Is there a direction you could look any clear night, no matter what time of year, and always see the same stars? Yes! Circumpolar constellations do not rise or set, but appear to move in a series of circles around Polaris, the pole star. In the northern hemisphere, between 30 and 40 degrees North la ...
Distance, Size, and Temperature of a Star
Distance, Size, and Temperature of a Star

PowerPoint Presentation - Properties of Stars
PowerPoint Presentation - Properties of Stars

... a) How does parallax vary with distance of the pen from your face? b) Is this method useful for finding distances to very far away things? Why or why not? c) To measure a parallax, you need a baseline—the distance between observation points. In the activity, the baseline was the distance between you ...
Chapter 11 Review
Chapter 11 Review

... 16. Explain why the frozen debris found in the Oort Cloud, more than 50 000 AU away from the Sun, is still considered part of the solar system. ...
Wednesday, November 7, 2007
Wednesday, November 7, 2007

... • Also contains lower-mass stars, some surrounded by disks ...
Stars: some basic characteristics
Stars: some basic characteristics

UNIT 3 INPUT 2: Notes on Black Holes (BH): Process of Formation
UNIT 3 INPUT 2: Notes on Black Holes (BH): Process of Formation

... Event Horizon: Within a certain distance of singularity: gravitational pull  very strong  nothing (not even light) could escape. Characteristics: Not a physical boundary The point-of-no-return nothing (even light) could get out Size of black hole = Size of event horizon The more mass of singulari ...
PPT - McMaster Physics and Astronomy
PPT - McMaster Physics and Astronomy

... 4(1H )4He  2  energy Nuclear reactions yield predictable neutrino fluxes from the Sun that directly reflect reaction rates ...
Stellar Evolution - Harnett County High Schools Wiki
Stellar Evolution - Harnett County High Schools Wiki

... Density and temperature increase toward the center, where energy is generated by nuclear fusion (hydrogen into helium)  Stars not on main sequence either fuse different elements in their core, or do not undergo fusion at all ...
What is a Star
What is a Star

... hottest ones) blue. The brightness is measured in magnitude, the brighter the star the lower the magnitude. There are two ways to measure the brightness of a star, apparent magnitude is the brightness seen from Earth, and absolute magnitude which is the brightness of a star seen from a standard dist ...
How are stars formed
How are stars formed

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Hipparcos



Hipparcos was a scientific satellite of the European Space Agency (ESA), launched in 1989 and operated until 1993. It was the first space experiment devoted to precision astrometry, the accurate measurement of the positions of celestial objects on the sky. This permitted the accurate determination of proper motions and parallaxes of stars, allowing a determination of their distance and tangential velocity. When combined with radial-velocity measurements from spectroscopy, this pinpointed all six quantities needed to determine the motion of stars. The resulting Hipparcos Catalogue, a high-precision catalogue of more than 118,200 stars, was published in 1997. The lower-precision Tycho Catalogue of more than a million stars was published at the same time, while the enhanced Tycho-2 Catalogue of 2.5 million stars was published in 2000. Hipparcos‍ '​ follow-up mission, Gaia, was launched in 2013.The word ""Hipparcos"" is an acronym for High precision parallax collecting satellite and also a reference to the ancient Greek astronomer Hipparchus of Nicaea, who is noted for applications of trigonometry to astronomy and his discovery of the precession of the equinoxes.
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