Astronomy Learning Objectives and Study Questions for Chapter 12
... B. red giant C. white dwarf D. blue-white supergiant E. supernova 6. The period during which an RR Lyrae or Cepheid variable star brightens and dims is directly related to its _____. A. distance B. temperature C. composition D. apparent magnitude E. absolute magnitude 7. Star clusters are important ...
... B. red giant C. white dwarf D. blue-white supergiant E. supernova 6. The period during which an RR Lyrae or Cepheid variable star brightens and dims is directly related to its _____. A. distance B. temperature C. composition D. apparent magnitude E. absolute magnitude 7. Star clusters are important ...
Irregular Galaxies
... • Supernovas can light up the sky for many weeks. • The core of the star becomes tremendously hot, fusing iron atoms into new elements. • Huge clouds of dust, gas, and the new elements explode into space. • This forms a new nebula. • Once a star supernovas, the core that remains of it will become ei ...
... • Supernovas can light up the sky for many weeks. • The core of the star becomes tremendously hot, fusing iron atoms into new elements. • Huge clouds of dust, gas, and the new elements explode into space. • This forms a new nebula. • Once a star supernovas, the core that remains of it will become ei ...
TU Muscae and the Early-type Overcontact Binaries
... Double-lined spectroscopic binary: spectral lines of both stars are visible. ...
... Double-lined spectroscopic binary: spectral lines of both stars are visible. ...
Chapter 5 Mid-term Study Guide
... Part A 1–8. Number the steps to show the sequence of a star’s life. Write the correct number on the line before each step. ______ A small star becomes a white dwarf, and a large star becomes a neutron star or black hole. ______ The star collapses again and then explodes as a nova or supernova. _____ ...
... Part A 1–8. Number the steps to show the sequence of a star’s life. Write the correct number on the line before each step. ______ A small star becomes a white dwarf, and a large star becomes a neutron star or black hole. ______ The star collapses again and then explodes as a nova or supernova. _____ ...
chap17_f03_phints
... luminosity 64X greater. What is this star’s radius, expressed in solar units ? HINT: Problem 4 is an application of the radius – luminosity – temperature relation for stars. Given two of these values, the third is found using that relation, described on pg 449 in the text. PROBLEM 10: Given a star w ...
... luminosity 64X greater. What is this star’s radius, expressed in solar units ? HINT: Problem 4 is an application of the radius – luminosity – temperature relation for stars. Given two of these values, the third is found using that relation, described on pg 449 in the text. PROBLEM 10: Given a star w ...
“Do you have a good caption for the pop-eyed, thin
... Centauri, famous for being the closest visible star, 4.3 light years away. The light left that star 4.3 years ago. At 186 thousand miles per second, the light traveled over 25 trillion miles from Alpha Centauri to reach Earth. Alpha Centauri means this star is the brightest star in the constellation ...
... Centauri, famous for being the closest visible star, 4.3 light years away. The light left that star 4.3 years ago. At 186 thousand miles per second, the light traveled over 25 trillion miles from Alpha Centauri to reach Earth. Alpha Centauri means this star is the brightest star in the constellation ...
REVIEW: STAR`S TEST
... Approximately 90% of the visible universe’s mass is composed of ___hydrogen___ In the H-R diagram, stars are classified on the basis of ...
... Approximately 90% of the visible universe’s mass is composed of ___hydrogen___ In the H-R diagram, stars are classified on the basis of ...
Chapter 30 Study Notes
... A star with the sun’s mass would stay on the main sequence of the H-R diagram for about _____ 10 billion years. ...
... A star with the sun’s mass would stay on the main sequence of the H-R diagram for about _____ 10 billion years. ...
March
... Galaxy for it’s elongated shape, M82 is also about 12 million Light Years distant. The close encounter with M81 described above distorted the shape of this irregular galaxy, creating many bright, turbulent star-forming regions. Over 100 globular clusters have been observed orbiting this galaxy. NGC ...
... Galaxy for it’s elongated shape, M82 is also about 12 million Light Years distant. The close encounter with M81 described above distorted the shape of this irregular galaxy, creating many bright, turbulent star-forming regions. Over 100 globular clusters have been observed orbiting this galaxy. NGC ...
Ch. 28 Test Topics
... -Know that this is the order of objects in the universe from smallest to largest: planet, solar system, star, star cluster, galaxy, galaxy cluster, super cluster -Know a local group of galaxies are galaxies that are in the close by each other and in our galaxy cluster. The other galaxies in our loca ...
... -Know that this is the order of objects in the universe from smallest to largest: planet, solar system, star, star cluster, galaxy, galaxy cluster, super cluster -Know a local group of galaxies are galaxies that are in the close by each other and in our galaxy cluster. The other galaxies in our loca ...
Constellation Information
... supergiant that pours out about 50,000 times as much light as out Sun. Most of Orions main stars, roughly 1,400 light-years away. Betelgeuse is nearer at about 500 light-years. Orion holds (what some consider the most magnificent telescopic sight beyond our solar system) M42, the Great Orion Nebula ...
... supergiant that pours out about 50,000 times as much light as out Sun. Most of Orions main stars, roughly 1,400 light-years away. Betelgeuse is nearer at about 500 light-years. Orion holds (what some consider the most magnificent telescopic sight beyond our solar system) M42, the Great Orion Nebula ...
Physical properties of stars
... Absolute magnitude depends on: The size of the star The temperature of the star Apparent magnitude depends on: The size of the star The temperature of the star The distance of the star Pg. 444 scale of objects and their apparent magnitude. Absolute motion- the actual motion of stars in spa ...
... Absolute magnitude depends on: The size of the star The temperature of the star Apparent magnitude depends on: The size of the star The temperature of the star The distance of the star Pg. 444 scale of objects and their apparent magnitude. Absolute motion- the actual motion of stars in spa ...
PowerPoint File
... Measure the distance over which the density of stars significantly falls off with height above, or distance below, the galactic plane. The distance depends on the type of objects considered, but is roughly 100 – 200 parsecs. The galactic plane is much thinner than it is wide. ...
... Measure the distance over which the density of stars significantly falls off with height above, or distance below, the galactic plane. The distance depends on the type of objects considered, but is roughly 100 – 200 parsecs. The galactic plane is much thinner than it is wide. ...
chapter 18
... uranium to form lead, Pb. b) helium nuclei to form carbon nuclei. c) hydrogen nuclei to form helium nuclei. d) carbon nuclei to form magnesium nuclei. ...
... uranium to form lead, Pb. b) helium nuclei to form carbon nuclei. c) hydrogen nuclei to form helium nuclei. d) carbon nuclei to form magnesium nuclei. ...
A Star’s Life
... 1. Read the two life cycle assignments (part I and II). 2. Create a graphic organizer that summarizes what you are reading. 3. Check your answers to the questions of part I (summary questions at the end) and part II (sections 1, 2, 4 and 5) in schoology. Note: the true/false section (Those A-Maz-Ing ...
... 1. Read the two life cycle assignments (part I and II). 2. Create a graphic organizer that summarizes what you are reading. 3. Check your answers to the questions of part I (summary questions at the end) and part II (sections 1, 2, 4 and 5) in schoology. Note: the true/false section (Those A-Maz-Ing ...
18-3 constellations RG
... ______________________________________________________________ 3. What is the name of the constellation pictured above, and how did the ancient Greeks and Japanese view it differently? See figure 1 on page 564 ______________________________________________________________ ___________________________ ...
... ______________________________________________________________ 3. What is the name of the constellation pictured above, and how did the ancient Greeks and Japanese view it differently? See figure 1 on page 564 ______________________________________________________________ ___________________________ ...
Lecture4
... A star cluster of 10,000 stars all formed at the same QuickTime™ and a time. The HR diagram evolving with time. YUV420 codec decompressor are needed to see this picture. ...
... A star cluster of 10,000 stars all formed at the same QuickTime™ and a time. The HR diagram evolving with time. YUV420 codec decompressor are needed to see this picture. ...
Characteristics of Stars
... Stars that glow blue-white are the hottest (15,000 degrees Celsius) Rigel ...
... Stars that glow blue-white are the hottest (15,000 degrees Celsius) Rigel ...
Serpens
Serpens (""the Serpent"", Greek Ὄφις) is a constellation of the northern hemisphere. One of the 48 constellations listed by the 2nd-century astronomer Ptolemy, it remains one of the 88 modern constellations defined by the International Astronomical Union. It is unique among the modern constellations in being split into two non-contiguous parts, Serpens Caput (Serpent's Head) to the west and Serpens Cauda (Serpent's Tail) to the east. Between these two halves lies the constellation of Ophiuchus, the ""Serpent-Bearer"". In figurative representations, the body of the serpent is represented as passing behind Ophiuchus between Mu Serpentis in Serpens Caput and Nu Serpentis in Serpens Cauda.The brightest star in Serpens is the red giant star Alpha Serpentis, or Unukalhai, in Serpens Caput, with an apparent magnitude of 2.63. Also located in Serpens Caput are the naked-eye globular cluster Messier 5 and the naked-eye variables R Serpentis and Tau4 Serpentis. Notable extragalactic objects include Seyfert's Sextet, one of the densest galaxy clusters known; Arp 220, the prototypical ultraluminous infrared galaxy; and Hoag's Object, the most famous of the very rare class of galaxies known as ring galaxies.Part of the Milky Way's galactic plane passes through Serpens Cauda, which is therefore rich in galactic deep-sky objects, such as the Eagle Nebula (IC 4703) and its associated star cluster Messier 16. The nebula measures 70 light-years by 50 light-years and contains the Pillars of Creation, three dust clouds that became famous for the image taken by the Hubble Space Telescope. Other striking objects include the Red Square Nebula, one of the few objects in astronomy to take on a square shape; and Westerhout 40, a massive nearby star-forming region consisting of a molecular cloud and an H II region.