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TE SC.4.E.5.4, 5.3, 5.2, 5.1
TE SC.4.E.5.4, 5.3, 5.2, 5.1

The Origin, Structure, and Evolution of the Stars
The Origin, Structure, and Evolution of the Stars

October 2014 - Hermanus Astronomy
October 2014 - Hermanus Astronomy

... The NASA Kepler space telescope has confirmed about 1,000 exoplanets, as well as thousands of more stars considered ‘Kepler objects of interest’, dubbed KOIs stars that could possibly host planets. Until now, there has been an unanswered question about exoplanet host stars: How many host stars are b ...
Life Stages of High
Life Stages of High

... Planetary Nebulae • Double-shell burning ends with a pulse that ejects the H and He into space as a planetary nebula • The core left behind becomes a white dwarf ...
Slide 1
Slide 1

... accretion disk indicating BH or WH in center--a quadrillion solar masses!) The Pisces-Cetus Complex: may include 400 rich (and lots of poor) clusters. Brent Tully. Is the Universe homogeneous? God's Bubble Bath: Galaxy superclusters seem to from in bubble structures and filaments with Voids 100-500 ...
Testing
Testing

... our view because they absorb visible light. This is the interstellar medium that makes new star systems. ...
Orion – The Hunter - Guild of Students
Orion – The Hunter - Guild of Students

... the scorpion in the night sky as the constellations Orion and Scorpius. She placed the scorpion opposite him, so that never are the two visible at once. The sky shows him followed by his two fighting dogs, Canis Major and Minor, and fighting a bull, Taurus. Oddly, the bull is completely irrelevant t ...
sections 12-15 instructor notes
sections 12-15 instructor notes

... the University of Toronto, April 1979) Luminosity Functions. Every astronomer deals almost daily with luminosity functions of some sort. In a way the most basic of such functions is the general luminosity function (GLF), which gives us the distribution function of absolute magnitude, M, for the aver ...
The Death of a Star
The Death of a Star

... under so much pressure at this time that fusion is no longer possible. This incredible amount of pressure is enough to force the electrons to react with the protons turning them all into neutrons. Without the outward resistance of the electrons the core collapses to about 50 km in radius. The amount ...
A-level Physics A Mark scheme Unit 05 - Section 2A
A-level Physics A Mark scheme Unit 05 - Section 2A

... relevant questions, by a panel of subject teachers. This mark scheme includes any amendments made at the standardisation events which all associates participate in and is the scheme which was used by them in this examination. The standardisation process ensures that the mark scheme covers the studen ...
FantasticTrip - Cooper Church of Christ
FantasticTrip - Cooper Church of Christ

... of the ends of the earth, And the wicked be shaken out of it? 14 It takes on form like clay under a seal, And stands out like a garment. 15 From the wicked their light is withheld, And the upraised arm is broken. 16 "Have you entered the springs of the sea? Or have you walked in search of the depths ...
AQA Minutes Template
AQA Minutes Template

... relevant questions, by a panel of subject teachers. This mark scheme includes any amendments made at the standardisation events which all associates participate in and is the scheme which was used by them in this examination. The standardisation process ensures that the mark scheme covers the studen ...
Spectral Classification of Stars
Spectral Classification of Stars

PDF - Interactive Stars
PDF - Interactive Stars

... Great Bear, at all, but Philomelus, 'the lover of song', who was the son of Demeter, the 'law-giver' and the goddess of the harvest and the corn. Philomelus was the inventor of the wagon, for which he was immortalised amongst the stars, according to this version of the story, and from which the cons ...
File
File

9. Fascinating observations. But how much is well understood?
9. Fascinating observations. But how much is well understood?

... primary star. In HMXB systems the normal star is often of spectral type B, a hot very luminous star with several times the solar radius. The orbital period is a few weeks till months. The B-star has an effective temperature between 1 − 3 ⋅ 10 4 K and masses M > 10M sol . B-stars rotate rapidly and e ...
Armillary Sphere (1:1)
Armillary Sphere (1:1)

... է ʟ nigh Mi ...
Warm up to the Solar System`s Furnace
Warm up to the Solar System`s Furnace

The Formation of Massive Star Systems by Accretion
The Formation of Massive Star Systems by Accretion

Planets in different environments
Planets in different environments

Evolved Stellar Populations
Evolved Stellar Populations

... Magellanic Clouds data  The MCs are an example of interacting Irr galaxies like others in the Universe.  Previous results were obtained from spatially limited regions in the outer/inner disk and in the bar (i.e. using HST). No global picture!  Wide-field observations:  Near-IR DENIS & 2MASS (on ...
Theme 7.2 -- The Complete Solar System
Theme 7.2 -- The Complete Solar System

ppt
ppt

... Cloud and star formation may have to be treated together Both magnetic and non-magnetic turbulence simulations are promising  Observations of the large scale magnetic field strength are needed to ...
How Big Is Our Universe? - Harvard
How Big Is Our Universe? - Harvard

No. 35 - Institute for Astronomy
No. 35 - Institute for Astronomy

< 1 ... 108 109 110 111 112 113 114 115 116 ... 393 >

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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