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Data Visualization
Data Visualization

... Reduce number of variables, preserve information Principal Component Analysis – Transform to new coordinate system – Hard to interpret ...
Magnetic fields in O-, B-and A-type stars on the main sequence
Magnetic fields in O-, B-and A-type stars on the main sequence

... Massive stars have thin sub-surface convective layers that are induced by the iron opacity bump near the surface. Therefore, it is plausible that a dynamo process can operate in the sub-surface convection zones. Moreover, these fields could reach the stellar surface and it is shown that increasing s ...
The masses of stars
The masses of stars

... brightness of stars, known as their magnitude. This measurement scale was originally devised by Hipparchus, a 2nd Century BC Greek astronomer who introduced it as a system to compare the brightness of different stars: the very brightest stars that could be seen with the unaided eye were labelled ‘fi ...
12.1 Introduction
12.1 Introduction

... The evolution of more massive stars on the main sequence differs from that of solar mass stars in one important aspect: stars more massive than the Sun have convective cores, as we saw in Lecture 8.3.1. The timescale for convection, defined as the time it takes for a convective element to travel one ...
Death of Stars • Models of Star behavior can give estimates of how
Death of Stars • Models of Star behavior can give estimates of how

... Will see that this also gets used as a way to see how far away a star is. White Dwarves • Again, these are the remainders of stars that could not proceed any further because they could not raise their internal temperatures high enough to fuse the remaining elements. • Dense hot balls of Carbon (or H ...
Seeds of a Tychonic Revolution: Telescopic Observations of the
Seeds of a Tychonic Revolution: Telescopic Observations of the

... scattered throughout space, so such a pair must be in line-of-sight alignment. However, at the distances implied by Mareo's hypothesis, these two stars should exhibit parallax if the Earth is moving, and the difference between the parallaxes of the two stars (differential parallax) must greatly exce ...
Folie 1
Folie 1

... The total abundance of C, N, O (and F) nuclei is constant in time ...
Ptolemy: on trial for fraud
Ptolemy: on trial for fraud

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Slug: Meteor Shower On me
Slug: Meteor Shower On me

base text pdf - Max-Planck
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The Life Cycle of Stars
The Life Cycle of Stars

... to the pull of gravity. The core temperature rises until it meets a critical temperature of 15 million °C (1.5 × 107 °C). At this temperature, nuclear fusion begins. Hydrogen atoms in the core fuse to form helium atoms, producing an enormous amount of energy. This energy rushes outward from the core ...
Phys 214. Planets and Life
Phys 214. Planets and Life

... surprise and is forcing theorists to revise their understanding of how young planetary systems evolve. According to our current theory of planet formation, Jupiter-like planet cannot form close to its parent star because it would be too hot for gases to condense. However, they can form farther out a ...
SGHS Faulkes ASISTM Star Cluster Photometry
SGHS Faulkes ASISTM Star Cluster Photometry

... B and V images. Note: When you complete this you will see that the spreadsheet has calculated a B-V value for each star. i) Now you need to repeat the process for the open cluster NGC2420. The images we will use are NGC2420-B.fits and NGC2420-V.fits. You will see there is a sheet in the Excel spread ...
CONSTELLATIONS
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The Milky Way Galaxy
The Milky Way Galaxy

... spheroid. A massive black hole marks the center of the Galaxy. The (Our) Sun sits far out in the disc and in visible light. Our view of the Galaxy is limited by interstellar dust. Consequently, the large-scale structure of the Galaxy must be inferred from observations made at infrared and radio wave ...
Design a Space Telescope - Herschel Space Observatory
Design a Space Telescope - Herschel Space Observatory

... 3) A university has approached your group to design a mission for satellite telescope in order to analyse the spectra of interstellar dust in nearby galaxies. The budget of your mission is £9 billion. You will need the appropriate instruments on board the telescope in order to carry out the mission. ...
www.astro.org.uk www.facebook.com/Stra ordAstro www.twi er.com
www.astro.org.uk www.facebook.com/Stra ordAstro www.twi er.com

... Explorer 1 and its multi-stage launch system was designed by von Braun. ...
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Lecture 4: Telescopes

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August 2014 Saguaro Skies
August 2014 Saguaro Skies

... Aquarius. First is Sagitta and an open cluster that probably isn’t on many observing lists. It is Harvard 20 and since it isn’t that well known here are the coordinates RA 19 53.1 Dec +18 21. It is in a rich Milky Way field and doesn’t stand out well so a finder chart would be helpful. Next is the g ...
Cosmological Aspects of Nucleosynthesis
Cosmological Aspects of Nucleosynthesis

... Formed during quiescent phases of stellar evolution: He-burning in AGB stars and massive stars ...
Journey to the Stars Educator`s Guide
Journey to the Stars Educator`s Guide

... observational techniques to see small, dim objects like brown dwarfs. On Earth and in space, these telescopes are our eyes to the universe. ...
30 Doradus - HubbleSOURCE
30 Doradus - HubbleSOURCE

... 1. Gigantic regions of star formation are complex systems where different generations of star affect each other’s evolution 2. At high redshift we cannot see the complexity of the star forming regions, and we derive a simplified history of star formation 3. A comparison between what we see in nearby ...
Neil F. Comins - Kuwait Life Sciences Company
Neil F. Comins - Kuwait Life Sciences Company

... discovery and interpretation. Dozens of these conceptdriven, experiential walkthroughs allow students to make observations, draw conclusions, and apply their knowledge. Interwoven with multimedia, activities, and questions, students receive a deep, self-guided exploration of the concepts. ...
DSLR Photometry
DSLR Photometry

... Tricks and Shortcuts The preceding is complex and involved, but necessary for the highest accuracy and precision. Computers simplify the process. More details of the foregoing can be found in the book AutoStar CCD Photometry. With CCD (DSLR) photometry, if the program and comparison star are close ...
Study Island
Study Island

... 3. A prediction is a forecast about what may happen in some future situation. An inference is an explanation based on observations and background knowledge. Based on these definitions, which of the following statements is a prediction? A. The stove was hot because the kitchen light was on too long. ...
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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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