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black hole
black hole

... This wobble may be caused by the combined gravitational pull of two planets with 67 and 98 day orbital periods. ...
AY5 Announcements
AY5 Announcements

... •  For stars less than 8Mo these last slides describe the evolution pretty well. There are some differences in the details that depend on the initial main-sequence mass. •  For stars that start with 4Mo, it gets hot enough in the cores to ignite start carbon fusion on the main sequence. •  The WD re ...
Assignment 7 - Department of Physics and Astronomy
Assignment 7 - Department of Physics and Astronomy

... ____ 19. Stars that do not have what it takes to succeed as a star (i.e. do not have enough mass to fuse hydrogen into  helium at their centers) are called: a. extras b. red giants c. spectroscopic stars d. brown dwarfs e. main sequence stars ____ 20. Which of the following has the smallest mass? a ...
ASTR 1120 General Astronomy: Stars and Galaxies
ASTR 1120 General Astronomy: Stars and Galaxies

section 17 powerpoint
section 17 powerpoint

... by 1 Astronomical Unit, A.U., at the distance of a star. In practice one can observe the annual displacement of a star resulting from Earth’s orbit about the Sun as 2π. Since all stars should exhibit parallax, measured values (trigonometric parallaxes) are of two types: πrel = relative parallax, is ...
H-R Diagram
H-R Diagram

... 3. Organize: Select Mass from the Arranged by menu. Position the stars on the Gizmo’s mass scale, and mark these positions on the scale below. (Remember to click Sort stars to check ...
Star Formation
Star Formation

HEA_Accretion_2003_04
HEA_Accretion_2003_04

... disk is disrupted in inner parts. Material is channeled along field lines and falls onto star at magnetic poles ...
The portion of light we detect from a star/blackbody depends on
The portion of light we detect from a star/blackbody depends on

... We can spread the light of a star out into its component colors. We find that these spectra fall into three categories: ...
Exoplanet, 51 Pegasi b, Solar System, VLT, La Silla. ESOcast
Exoplanet, 51 Pegasi b, Solar System, VLT, La Silla. ESOcast

... richest planetary system yet. The system, located over 120 light-years away around the Sun-like star HD 10180, contains at least five exoplanets. There is also tantalising evidence that two more planets may be present in this system, one of which would have the lowest mass ever found. ...
Star Finder
Star Finder

Dark Sky Scotland - Constellation Project
Dark Sky Scotland - Constellation Project

... Centauri and even this close neighbour is about four Light Years away! In 1838, Thomas Henderson, Astronomy Royal for Scotland, was one of three scientists who, independently, first measured the distances to nearby stars. This helped to provide a dramatically new appreciation of the scale of the Uni ...
AST 1010 Quiz questions
AST 1010 Quiz questions

... 1. Explain why the Moon goes through a series of phases. Be sure to include a description of how the relative positions of the Sun, Moon and Earth affect this process. 2. Explain why most locations on the Earth experience a cycle of seasons. Be sure to be specific as to which hemisphere you are desc ...
The correct answers are written in bold, italic and underlined. The
The correct answers are written in bold, italic and underlined. The

... 15. Tritium is a radioactive form of hydrogen in which the nucleus contains one proton and two neutrons. How much more massive is this nucleus than that of ordinary hydrogen? • The same mass because this nucleus is still hydrogen • Three times as massive • Twice as massive 16. Electron transitions b ...
Hunting for Extrasolar Planets: Methods and Results
Hunting for Extrasolar Planets: Methods and Results

Measuring the Milky Way
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... Variable stars provide a better way to measure distances. Stars whose luminosity varies in a regular way are called intrinsic variables. Two types of intrinsic variables have been found: RR Lyrae stars, and Cepheids. ...
Meet the Jovians` Hot Siblings DONT ERASE
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... • While Jupiter is 5.3 AU away from its parent star, TrES-4b is 0.053 AU away from its parent star. ...
Merak
Merak



... 3. THE RR LYRAE STARS IN M15 In Clement’s (2002) data base of variables stars, a total of 158 variable stars are known, from which approximately 104 are RR Lyrae type stars. In this work, 33 known RR Lyrae stars, identified in Figs. 1 and 2 and listed in Table 4, have been studied. For all the stars ...
(a) Because the core of heavy-mass star never reaches high enough
(a) Because the core of heavy-mass star never reaches high enough

... (d) IV is a main sequence star (e) V is a brown dwarf Answer (d) 5. What is the smallest mass a newborn star can have? (a) 8.00 × Msun (b) 0.8 × Msun (c) 0.08 × Msun (d) 0.008 × Msun (e) 0.0008 × Msun Answer (c) 6. Which one of the following does not belong in the life and death of a high-mass star? ...
MS PowerPoint - National Schools` Observatory
MS PowerPoint - National Schools` Observatory

... well if you get within 2 light-years of that value. Velocity : The official value is around 90 km/sec, but again, if you get within 20% of that figure, then you are doing very well. Don’t forget, this is only the velocity perpendicular (sideways) to our line of sight. So, by combining simple measure ...
E8B6_CRT_CR_MSTIPS_Final
E8B6_CRT_CR_MSTIPS_Final

Stars on the HR Diagram
Stars on the HR Diagram

... 2. Use one colored pencil to plot the nearest stars, 15 light years from the sun or closer, and another color for the stars that are more than 15 light years from the sun. Alternative method – attach chart to foam or cardboard backing and use 2 colors of push pins to mark the stars. 3. With a 3rd co ...
Solutions
Solutions

... by the newly formed OB Association stars that emit most of their energy as high-energy short-wavelength hardUV photons. The photons from the OB Association stars “power up” the HII region and keep it fluorescing. Thus the OB Association forms first and then the HII region is created around the vicin ...
Planetary Configurations
Planetary Configurations

... Suppose a gas giant lies in the habitable zone. Although unlikely to support life, perhaps one of its moons could. ...
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Lyra



Lyra (/ˈlaɪərə/; Latin for lyre, from Greek λύρα) is a small constellation. It is one of 48 listed by the 2nd century astronomer Ptolemy, and is one of the 88 constellations recognized by the International Astronomical Union. Lyra was often represented on star maps as a vulture or an eagle carrying a lyre, and hence sometimes referred to as Aquila Cadens or Vultur Cadens. Beginning at the north, Lyra is bordered by Draco, Hercules, Vulpecula, and Cygnus. Lyra is visible from the northern hemisphere from spring through autumn, and nearly overhead, in temperate latitudes, during the summer months. From the southern hemisphere, it is visible low in the northern sky during the winter months.The lucida or brightest star—and one of the brightest stars in the sky—is the white main sequence star Vega, a corner of the Summer Triangle. Beta Lyrae is the prototype of a class of stars known as Beta Lyrae variables, binary stars so close to each other that they become egg-shaped and material flows from one to the other. Epsilon Lyrae, known informally as the Double Double, is a complex multiple star system. Lyra also hosts the Ring Nebula, the second-discovered and best-known planetary nebula.
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