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Stars
Stars

... determines the extent to which material from the deep interior of the star is mixed into the outer layers. Since interior material is likely to have undergone nuclear reactions, which change the elemental abundances, this mixing affects the abundances in the star's atmosphere. These can be observed ...
Sun - Midlandstech
Sun - Midlandstech

... pole follows a circular pattern on the sky, once every 26,000 years. It will be closest to Polaris ~ A.D. 2100. There is nothing peculiar about Polaris at all (neither particularly bright nor nearby etc.) ...
Chapter 1 - A Modern View of the Universe
Chapter 1 - A Modern View of the Universe

... shines by reflected optical light from its host star. Planets may be rocky or gaseous in composition. ...
May 2013 - Otterbein
May 2013 - Otterbein

... Some look blue, some red Some live shorter, others longer Some end up as black holes, some as neutron stars, some as white dwarfs ...
Investigate Stars and Galaxies - American Museum of Natural History
Investigate Stars and Galaxies - American Museum of Natural History

The life of Stars
The life of Stars

... Mira Stars • Mira (=wonderful, lat.) [o Ceti]: sometimes visible with bare eye, sometimes faint • Long period variable star: 332 days period • Cool red giants • Sometimes periodic, sometimes irregular • some eject gas into space ...
April 1st
April 1st

... When does a protostar become a star • When the core temperatures reaches 10 million K, hydrogen fusion can start occurring ...
DSLR photometry - British Astronomical Association
DSLR photometry - British Astronomical Association

Phys 100 – Astronomy (Dr. Ilias Fernini) Review Questions for
Phys 100 – Astronomy (Dr. Ilias Fernini) Review Questions for

Which of the following statements is TRUE
Which of the following statements is TRUE

... Studies of the Cosmic Microwave Background Radiation allow us to probe the properties of the Universe all the way back to Big Bang ...
DO NOW - PBworks
DO NOW - PBworks

... **Teacher will model how to do this** 2. For each star, put an “X” next to the element name for each element it has on RM 21. ...
Stellar Life Stages
Stellar Life Stages

... use up their hydrogen and collapse into a white dwarf ...
stars
stars

... • Numbers varies in cycles, with about 11 years separating one sunspot peak from the next. ...
Spectroscopic Investigation of Companion Stars in Herbig
Spectroscopic Investigation of Companion Stars in Herbig

... Anne Sweet1, B. Rodgers2, G. Doppmann2, N. van der Bliek3, S. Thomas3, M. J. Cordero1 1CTIO REU, Chile, 2Gemini Observatory, Chile, 3CTIO, Chile. Abstract Herbig AeBe (HAEBE) binary systems are good environments for the study of pre-main sequence stellar evolution in companion stars whose mass may b ...
There are 88 constellations in the sky around the Earth. 12 are the
There are 88 constellations in the sky around the Earth. 12 are the

... Australis (Delta Cancri), magnitude 3.9; Iota Cancri, magnitude 4.0; Acubens (Alpha Cancri), magnitude 4.2; Asellus Borealis (Gamma Cancri), magnitude 4.7 Noteable doubles are: Zeta Cancri, magnitudes 5.6 & 6.0 (A binary with separation 1 second of arc & a period of 60 years. Larger telescopes revea ...
Observing the Night Sky - Constellations
Observing the Night Sky - Constellations

Today`s Powerpoint
Today`s Powerpoint

... Luminosity = (energy radiated per cm2 per sec) x (area of surface in cm2) So: Luminosity  (temperature) 4 x (surface area) Determine luminosity from apparent brightness and distance, determine temperature from spectrum (black-body curve or spectral lines), then find surface area, then find radius ( ...
Discussion Activity #11a
Discussion Activity #11a

Unit I – The Size, Shape and Motion of the Earth
Unit I – The Size, Shape and Motion of the Earth

... moon, planets, asteroids, etc, to work out their distances and speeds. The stars are much too distant! (Any return signal would take years!) Moreover, the return signal would be much too feeble to detect. ...
Seating Chart for Wednesday PHOTO ID REQUIRED! SIT IN YOUR ASSIGNED ROW!
Seating Chart for Wednesday PHOTO ID REQUIRED! SIT IN YOUR ASSIGNED ROW!

... • Time slows down in strong grav. field…. even GPS systems are affected. ...
Untitled - New Zealand Science Teacher
Untitled - New Zealand Science Teacher

Bez tytułu slajdu
Bez tytułu slajdu

... The neutron ball is similar to a giant atomic nucleus with Z=1057. With such a big compression, neutrons start to "crowd-up", following the Pauli's rule, which does not allow them to be in the same quantum state. It is energetically useful to replace some neutrons with protons, or even by isolated q ...
Adventurer Pathfinder
Adventurer Pathfinder

... Sunspots are dark spots on the sun’s surface. Some spots are as large as 50,000 miles across and up to 2,000° cooler than the rest of the sun. These spots are caused by solar flares, or small explosions on the sun. Solar flares shoot energy into space. When the energy hits the earth, it causes magne ...
Star Life Cycle Web Activity
Star Life Cycle Web Activity

Astronomy Quiz #1 Answers
Astronomy Quiz #1 Answers

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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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