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The HIRES science case
The HIRES science case

... In general planets were thought to be mostly on orbits coplanar with their star's equator, something in line with predictions of disc migration. Recent results have shown that hot Jupiter planets on non-coplanar orbits are common, including some planets on retrograde orbits (Triaud et al. 2010). Tho ...
Solar System Formation
Solar System Formation

... circumstellar disk discovered by Koerner et al. (1998) … disk inclined by 72 deg emission intensity increases (!) with radius, implying inner hole 40-70 AU … clearance out to Kuiper Belt? ring width is < 17 AU from NICMOS observations … corresponding to thin Kuiper Belt, or shepherding planets? dust ...
Document
Document

Calculating Radial Velocities of Low Mass Eclipsing Binaries
Calculating Radial Velocities of Low Mass Eclipsing Binaries

... the same metallicity by assuming they were formed from the same material, so we get the metallicity for the M star from studying the primary star. Eclipsing binaries are classical two-body systems where two stars orbit each other around a ...
David`s Mapping the Heavens[1]
David`s Mapping the Heavens[1]

... 1 parsec is about 3x1013km ...
NIE10x301Sponsor Thank You (Page 1)
NIE10x301Sponsor Thank You (Page 1)

... for him but popular targets for astronomers ever since. Sir William Herschel (1738-1822) and other astronomers would turn larger and larger telescopes towards these catalogued “nebulosities” and discover many to have a generally circular, and often spiral-shaped, structure; they called these spiral ...
ASTRONOMY 301 EXAMPLES OF TEST
ASTRONOMY 301 EXAMPLES OF TEST

... north pole far from where it is now, it will no longer necessarily be warm in Hawaii and cold where the north pole is now. 15. If the plane of the Moon’s orbit around the Earth were the same as the plane of the Earth’s orbit around the Sun, there would be a total solar eclipse (A) (B) (C) (D) ...
Observers` Forum - British Astronomical Association
Observers` Forum - British Astronomical Association

... a complex area of fine filamentary structure inside the crescent which makes it look much more like a jellyfish than a crescent (the nebula is tilted to our line of sight by about 45°). Professional infrared images also show a much larger outer nebulous envelope. At the heart of the nebula is a Wolf ...
here. - Oswego
here. - Oswego

... • Airmass is the amount of atmospheric mass through which an observed signal passes. For small zenith angles, airmass = secz is a good approximation, where z is the zenith angle of the telescope (z = 0° when the telescope is pointed at the zenith, and z = 90° at the horizon). • At present, the airma ...
Constellations and the Galactic Plane
Constellations and the Galactic Plane

... Constellations are simply patterns of the brightest stars in the heavens that inspired the ancients to attribute names and stories to. Orion the hunter, Cygnus the swan, Leo the lion are all familiar names to northern hemisphere night sky watchers. There are 88 named constellations, each having nume ...
Sky, Celestial Sphere and Constellations
Sky, Celestial Sphere and Constellations

... So sky looks blue during the day, in fact what we see is the atmosphere illuminated by sunlight.. Light from stars are much less intense (weaker) than the scattered sun light from atmosphere, so we do not see them (unless a star happen to be very bright) Away from the atmosphere (in space, on moon…) ...
Mirrored Image Sep06.pub - High Desert Astronomical Society
Mirrored Image Sep06.pub - High Desert Astronomical Society

... were so many objects to look at, one hardly knew where to start. Neptune through Dave Meyer's Celestron 14” scope was a beautiful turquoise dot, very pretty. There were four 10” dobs, Dave Flowers, Cliff’s, Sue’s and Gary’s. Tony had his 12.5” Aldebaran dob and Gary his 16” truss dob. We had two gue ...
Lecture 7: Extrasolar Planets 01/08/2013 update: 725 exoplanets
Lecture 7: Extrasolar Planets 01/08/2013 update: 725 exoplanets

... Einstein's General Theory of Relativity. According to Einstein, when the light emanating from a star passes very close to another star on its way to an observer on Earth, the gravity of the intermediary star will slightly bend the light rays from the source star, causing the two stars to appear fart ...
ORBITAL MOTION
ORBITAL MOTION

... Stage 3. At densities of 1011 cm-3 and within a radius of 1014 cm the gas becomes opaque to the dust radiation even at 300microns. The energy released is trapped and the temperature rises. As the temperature ascends, the opacity also ascends. The core suddenly switches from isothermal to adiabatic. ...
Event Booklet - Exoplanets I Conference
Event Booklet - Exoplanets I Conference

September Globular Clusters - Salisbury Plain Observing Group
September Globular Clusters - Salisbury Plain Observing Group

Introduction - Beck-Shop
Introduction - Beck-Shop

Optical Astronomy Imaging Chain: Telescopes & CCDs
Optical Astronomy Imaging Chain: Telescopes & CCDs

... • flat field is what CCD would detect if uniformly illuminated ...
James`s 5-Page Final Exam Review
James`s 5-Page Final Exam Review

... 16) Zodiac. What is the Zodiac? a. The constellations around which the planets appear to orbit. b. The constellations through which the Moon appears to move through over the course of a month. c. The constellations through which the Sun appears to move through over the course of a year. d. The const ...
HW1-6
HW1-6

... changeable objects must be earthly. Since this star just suddenly appeared, the old system said it must be earthly (under the sphere of the moon). Tycho’s observations indicated that the star could not be close. If it were close, it would have shifted (parallax). ...
How to Plot the H-R Diagram and Use its Applications
How to Plot the H-R Diagram and Use its Applications

... There are seven main spectral type each letter of the alphabet has become known. Each subspectra, which are numbered from 0 to 90. Stars according to their spectral characteristics to be classified. Star from radiation spectrum analysis of the elements that show radiation of different wavelengths, c ...
WSN 42 (2016) 132-142
WSN 42 (2016) 132-142

... There are seven main spectral type each letter of the alphabet has become known. Each subspectra, which are numbered from 0 to 90. Stars according to their spectral characteristics to be classified. Star from radiation spectrum analysis of the elements that show radiation of different wavelengths, c ...
Low mass stars
Low mass stars

Slides from Dr. Frank`s Lecture17
Slides from Dr. Frank`s Lecture17

Stars and Light
Stars and Light

... • Material for problem about Kepler satellite was not adequately covered, so everyone was given 4 points for this problem. • Your answers, the answer key, and the test are all on ICON. • Office hours this Tuesday will be 1-2 pm. ...
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