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Watching Galaxies Form Near the Beginning of Time
Watching Galaxies Form Near the Beginning of Time

... • Galaxy spectra show a cutoff at 912 A due to absorption by neutral hydrogen • This allows a straightforward multicolor selection (blue in two bands, missing shortward of that) • Thousands of galaxies at z>2.7 have now been found in this way ...
Refusing to Go Quietly: GRBs and Their Progenitors
Refusing to Go Quietly: GRBs and Their Progenitors

... Advanced LIGO will be able to detect gravitational waves that stretch the length of the arms by a fraction of the size of a proton ...
Are Gamma-Ray Bursts good Star Formation Indicators?
Are Gamma-Ray Bursts good Star Formation Indicators?

Debris Belts around Vega - Astronomical Society of the Pacific
Debris Belts around Vega - Astronomical Society of the Pacific

... “Vega is wearing 2 belts!” (page 2 in this PDF) Debris Disk: a disk of small particles encircling a star or planet. “Belts,” “disks,” and “rings” are all debris disks. The Figure is the Herschel view of the whole system, where the star is very bright at the center The two solid circles mark radii of ...
FOURTH GRADE UNIVERSE - Math/Science Nucleus
FOURTH GRADE UNIVERSE - Math/Science Nucleus

Lab 1: The Celestial Sphere
Lab 1: The Celestial Sphere

Why Pluto Is Not a Planet Anymore or How Astronomical Objects Get
Why Pluto Is Not a Planet Anymore or How Astronomical Objects Get

File - metc instructors collab site
File - metc instructors collab site

Appendix - ClassZone
Appendix - ClassZone

Lecture 12: Galaxies View of the Galaxy from within Comparison to
Lecture 12: Galaxies View of the Galaxy from within Comparison to

... •  It has a disk about 25 kpc (80,000 ly) in radius and about 600 pc thick, with interstellar dust and gas strongly concentrated in the disk plane. •  The Sun orbits around the Galactic centre at a speed of about 220 km s-1. •  It takes about 220 million years to complete one orbit ...
Stars and the Milky Way
Stars and the Milky Way

... • The Sun is just one of the stars in the Milky Way. • It is called the Milky Way because when astronomers looked up at the sky, they saw a line of light that looked like some milk had been spilt. • Stars in our Milky Way can be white, yellow or red. White stars are the hottest and red are the coole ...
CHAPTER 6 THE CELESTIAL SPHERE
CHAPTER 6 THE CELESTIAL SPHERE

Neutron Star
Neutron Star

The Milky Way`s Spiral Arms
The Milky Way`s Spiral Arms

... • This compresses the interstellar clouds, triggering the formation of stars • The entire arm pattern rotates around the Milky Way once every 500 million years ...
Zodiac Party Game - Home - DMNS Galaxy Guide Portal
Zodiac Party Game - Home - DMNS Galaxy Guide Portal

The first cool rocky/icy exoplanet
The first cool rocky/icy exoplanet

... space-based (MPF) campaigns. The planets of our solar system are marked by yellow circles. While the larger velocity and the larger range of inclinations for which an eclipse can occur favour closer orbits for the radial-velocity and the transit technique, respectively, the astrometric signal increa ...
Chapter 2 User`s Guide to the Sky: Patterns and Cycles
Chapter 2 User`s Guide to the Sky: Patterns and Cycles

... Union (IAU) established 88 official constellations with clearly defined permanent boundaries that together cover the entire sky. •  A constellation now represents not a group of stars but a section of the sky—a viewing direction. •  Any star within the region belongs to only that one constellation. ...
Exploring the Stars in Orion – Light Year Madness!
Exploring the Stars in Orion – Light Year Madness!

Neutron Stars
Neutron Stars

... the radius of the sun, and collapses to a final radius of 0.01 R, what will its final angular speed become after the collapse? Assume the mass stays a constant. ...
29.1 Directed Reading Guide
29.1 Directed Reading Guide

α Centauri: a double star - University of Canterbury
α Centauri: a double star - University of Canterbury

... closest approach: ...
October 2016 BRAS Newsletter - The Baton Rouge Astronomical
October 2016 BRAS Newsletter - The Baton Rouge Astronomical

memphis astronomical society short course in astronomy 2015
memphis astronomical society short course in astronomy 2015

Stellar Properties
Stellar Properties

... inverse-square law ...
X-ray Emission Line Profile Diagnostics of Hot Star Winds
X-ray Emission Line Profile Diagnostics of Hot Star Winds

... Although there’s not good reason to think that these young O stars have convection or magnetic dynamos, they may have magnetic fields that remain from the the collapsing interstellar clouds out of which they formed In fact, q1 Ori C itself has recently had a magnetic field detected on it: A large s ...
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Ursa Minor



Ursa Minor (Latin: ""Smaller She-Bear"", contrasting with Ursa Major), also known as the Little Bear, is a constellation in the northern sky. Like the Great Bear, the tail of the Little Bear may also be seen as the handle of a ladle, hence the name Little Dipper. It was one of the 48 constellations listed by the 2nd-century astronomer Ptolemy, and remains one of the 88 modern constellations. Ursa Minor has traditionally been important for navigation, particularly by mariners, due to Polaris being the North Star.Polaris, the brightest star in the constellation, is a yellow-white supergiant and the brightest Cepheid variable star in the night sky, ranging from apparent magnitude 1.97 to 2.00. Beta Ursae Minoris, also known as Kochab, is an aging star that has swollen and cooled to become an orange giant with an apparent magnitude of 2.08, only slightly fainter than Polaris. Kochab and magnitude 3 Gamma Ursae Minoris have been called the ""guardians of the pole star"". Planets have been detected orbiting four of the stars, including Kochab. The constellation also contains an isolated neutron star—Calvera—and H1504+65, the hottest white dwarf yet discovered with a surface temperature of 200,000 K.
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