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... brick and cement (this is why you can get radio reception almost anywhere). Radio waves can also be picked up during the day so scientists can work at any time (optical telescopes can only be used at night.) Having such large waves requires a large object to read these waves. To the right is a radio ...
Orion - Starry Starry Night!
Orion - Starry Starry Night!

... Visible : Jan, Feb, Mar, Apr, Dec Winter - Spring Canis Major contains Sirius, the brightest star in the night sky, known as the "dog star". It is bright because of its proximity to our Solar System. In contrast, the other bright stars of the constellation are stars of great distance and high lumino ...
MODULE CODE: AHAN7024 TITLE: Heavenly Discourses DATED
MODULE CODE: AHAN7024 TITLE: Heavenly Discourses DATED

...  demonstrate a systematic understanding of the origins of zodiacs and constellations and the mapping of the sky in a variety of cultures;  critically evaluate representations and applications of celestial knowledge in literature, music and the visual arts;  display a sophisticated understanding o ...
Export To Word
Export To Word

... Response Template may help students organize their thoughts and make grading faster, but if you wish to focus on student writing skills, spelling, and grammar, then you may wish to have them respond in an essay without using the template. (51-90 min.) Once the students understand the instructions fo ...
ATA2010
ATA2010

... is in stars, so the dynamical theory is mostly stellar dynamics Following this basic descriptive introduction, I will go straight to the lectures on the theoretical dynamics. This will give you maximum opportunity to complete the assignments. We will then return to more advanced descriptive material ...
Lecture 15 Star Formation and Evolution 3/7
Lecture 15 Star Formation and Evolution 3/7

... the Be decays  slows up reaction Larger electric repulsion than p-p as larger electric charge (2 for He and 4 for Be). Therefore need about 100,000,000 degrees K for He burning  Stars like our Sun remain main sequence longer due to this PHYS 162 ...
Return Visit Optimization for Planet Finding
Return Visit Optimization for Planet Finding

... than another. For example, at V = 5 better results are consistently achieved when returning after 1 estimated orbital period than after 1/2 period. • While in some cases returning a fixed time after initial detection produces better results than basing the re-visit time on the approximated orbital p ...
The Milky Way Galaxy
The Milky Way Galaxy

Slide 1
Slide 1

... Confirm that Debye cooling occurs We can measure the Gamma of crystallization Low metallicity clusters may not produce significant O in cores of some of the 0.5Msun stars … or Brown and collaborators are right and Gamma = 230 - 260 • We find the first empirical evidence that Van Horn’s 1968 predicti ...
hubble_refurb
hubble_refurb

... The wispy, glowing, magenta structures in this image are the remains of a star 10 to 15 times the mass of the Sun that we would have seen exploding as a supernova 3,000 years ago. The remnant’s fast-moving gas is plowing into the surrounding gas of the galaxy, creating a supersonic shock wave in th ...
The evolution of stars - School of Physics
The evolution of stars - School of Physics

... underlying physical link between these properties. What is this link? For example, consider an alien scientist constructing a similar diagram ...
PowerPoint Presentation - color cara template
PowerPoint Presentation - color cara template

... CELT: 5 to 10, must be robust on an industrial scale Importance of systems engineering, industrial-strength hardening of all telescope components and systems ...
Measuring the Solar Diameter with a Michelson Radio
Measuring the Solar Diameter with a Michelson Radio

... of air in the turbulent atmosphere (d ∼ 10 cm), one can overcome the effect of seeing. The small aperture sizes ensure that the radiation wavefronts detected by each of the two telescopes are coherent, i.e., have approximately the same phase across each of the telescope apertures. The only ...
Shape of a slowly rotating star measured by asteroseismology
Shape of a slowly rotating star measured by asteroseismology

Molecular Outflows Driven by Young Brown Dwarfs And VLMs. New
Molecular Outflows Driven by Young Brown Dwarfs And VLMs. New

... edge-on situation could explain why MHO5 is so dim, and it could also explain the low radial (blue-shifted) velocity of the OI6300 line of ≈ 20 km/s. We downloaded this HIRES spectra from the Keck Observatory Archive (KOA), and the spectra were reduced using standard IRAF routines. This spectra was ...
Part I: Shining a Light on Visual Magnitude
Part I: Shining a Light on Visual Magnitude

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

... seek some of these celestial long term denizens this autumn, and get out under the night sky. ...
Time From the Perspective of a Particle Physicist
Time From the Perspective of a Particle Physicist

... • Stars “move” East to West over the course of one Night (in circle about the North Star) • Stars “move” East to West by 2 hours per month and “return” to the same position after one Year • It’s just caused by Earth’s daily spin and yearly orbit about the Sun • Star wheel depends on latitude: northe ...
Bayesian mass and age estimates for transiting exoplanet host stars⋆
Bayesian mass and age estimates for transiting exoplanet host stars⋆

Document
Document

...  You do have a textbook, and for most of your uncertainties with the various topics, reading the text will help! ...
CONTINUING GALACTIC FORMATION
CONTINUING GALACTIC FORMATION

... -There are tremendous quantities of radio signals emitted by the Milky Way's nucleus. -The immediate environment surrounding many hot blue stars. -Novae and Supernovae art frequent. -Observation of supergiant stars of short life times indicates that stars are being formed in the galactic center. -Th ...
exploring the solar system, the galaxies, and the
exploring the solar system, the galaxies, and the

... AND THE UNIVERSE WITH THE HUBBLE SPACE TELESCOPE This is an online pre-lab exercise designed to show you the resources for studying our universe that are available on the Hubble Telescope Web site, located at http://hubblesite.org. You will also link with the site Amazing Space (http://amazing-space ...
Exploring Space—The Universe: The Vast
Exploring Space—The Universe: The Vast

... formed as a result of a merger between two disk galaxies. 4. Review with students the life cycle of a star. How are stars formed? (A star is born when gravity pulls hydrogen gas from a nebula into a spinning cloud. The resulting nuclear reaction and nuclear fusion keep the star evolving.) How old is ...
main sequence stars of a open cluster
main sequence stars of a open cluster

... Draw CM diagram of an open cluster, and find out the main sequence. 2. Outline Take apparent magnitude of stars on the vertical axis, and take color (or spectral type) on the horizontal axis. The plot with these axes is called CM (or HR) diagram. In this work, draw CM diagram of an open cluster NGC ...
Chemical Composition and Evolutionary Status of the Ap Star HD
Chemical Composition and Evolutionary Status of the Ap Star HD

... Using the ATLAS9 code (Kurucz 1993), we computed a grid of model atmospheres with a metallicity of +0.5 for effective temperatures from 8100 to 8400 K (with a 100-K step) and surface gravities from 3.5 to 4.0 (with a 0.1 step). We then used the Synth3 code (Kochukhov 2007) to compute a series of synt ...
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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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