• Study Resource
  • Explore Categories
    • Arts & Humanities
    • Business
    • Engineering & Technology
    • Foreign Language
    • History
    • Math
    • Science
    • Social Science

    Top subcategories

    • Advanced Math
    • Algebra
    • Basic Math
    • Calculus
    • Geometry
    • Linear Algebra
    • Pre-Algebra
    • Pre-Calculus
    • Statistics And Probability
    • Trigonometry
    • other →

    Top subcategories

    • Astronomy
    • Astrophysics
    • Biology
    • Chemistry
    • Earth Science
    • Environmental Science
    • Health Science
    • Physics
    • other →

    Top subcategories

    • Anthropology
    • Law
    • Political Science
    • Psychology
    • Sociology
    • other →

    Top subcategories

    • Accounting
    • Economics
    • Finance
    • Management
    • other →

    Top subcategories

    • Aerospace Engineering
    • Bioengineering
    • Chemical Engineering
    • Civil Engineering
    • Computer Science
    • Electrical Engineering
    • Industrial Engineering
    • Mechanical Engineering
    • Web Design
    • other →

    Top subcategories

    • Architecture
    • Communications
    • English
    • Gender Studies
    • Music
    • Performing Arts
    • Philosophy
    • Religious Studies
    • Writing
    • other →

    Top subcategories

    • Ancient History
    • European History
    • US History
    • World History
    • other →

    Top subcategories

    • Croatian
    • Czech
    • Finnish
    • Greek
    • Hindi
    • Japanese
    • Korean
    • Persian
    • Swedish
    • Turkish
    • other →
 
Profile Documents Logout
Upload
Slide 1
Slide 1

... arXiv:1106.3131 Denis A. Leahy, Sharon M. Morsink and Yi Chou The accreting millisecond pulsar XTE J1807-294 is studied through a pulse-shape modeling analysis. The model includes blackbody and Comptonized emission from the one visible hot spot and makes use of the Oblate Schwarzschild approximation ...
Lecture12
Lecture12

... E. A white dwarf ...
newsletter - Thanet Astronomy Group
newsletter - Thanet Astronomy Group

Doppler Effect
Doppler Effect

... Astronomers can calculate the speed from the wavelength difference. ...
Chap 11 Characterizing Stars v2
Chap 11 Characterizing Stars v2

... nearer stars can be determined by stellar parallax, which is the apparent shift of a star’s location against the background stars while Earth moves along its orbit around the Sun. The distances to more remote stars are determined using spectroscopic parallax. The apparent magnitude of a star, denote ...
The Milky Way
The Milky Way

... –6 Short answer/problem questions (5 points each) –Equation sheet (10 points) ...
Making Visual Estimates
Making Visual Estimates

... brightness seemed about half way between two stars that were known to be magnitudes 5.0 and 6.0, what is the magnitude of the variable star? Crab Nebula (C. Pullen) ...
Word doc - UC-HiPACC - University of California, Santa Cruz
Word doc - UC-HiPACC - University of California, Santa Cruz

... What made this burst different from most others is that the sheer power of the explosion so comparatively nearby allowed astronomers to follow the star’s decline in brightness over many wavelengths for weeks, giving them a glimpse into details of the explosion’s physics usually too faint to observe. ...
Stars - cayugascience
Stars - cayugascience

D1 Stellar quantities (PPT)
D1 Stellar quantities (PPT)

... Despite the difficulties in assessing whether stars exist singly or in groups of two or more, it is thought that around fifty per cent of the stars nearest to the Sun are part of a star system comprising two or more stars. Binary stars consist of two stars that rotate about a common centre of mass. ...
005 Astrophysics problems
005 Astrophysics problems

... 10. (a) Explain what is meant by the term ‘escape velocity’. (b) Derive an expression for the escape velocity in terms of the mass and radius of a planet. (c) (i) Calculate the escape velocity from both the Earth and from the Moon. (ii) Using your answers to (i) comment on the atmosphere of the Eart ...
Lecture 20: Formation of Planets, Exoplanets 3/30
Lecture 20: Formation of Planets, Exoplanets 3/30

... -water may be trapped at beginning in dust grains or come later from comets hitting surface??? • further from star: Gas Giants ices (water H2O, methane CH4) froze out early  larger protoplanets  more material to accrete • comets, meteors, asteroids give clues to composition of early solar system ...
File
File

... *Arab astronomers saw one in AD 1006. *The Chinese saw one in AD 1054. *European astronomers observed two—one in AD 1572 (Tycho’s supernova) and one in AD 1604 (Kepler’s ...
Falling Stars
Falling Stars

... The sight of a falling star is always exciting. Before the word “look!” is out of your mouth, the streak of light is gone. You point to where it was and ask others if they saw it, too. Often, no one else sees the speedy flight of light flash by, and you are left trying to describe what you saw and f ...
Doppler Effect
Doppler Effect

r*=13.6 km MPA1 EOS
r*=13.6 km MPA1 EOS

... arXiv:1106.3131 Denis A. Leahy, Sharon M. Morsink and Yi Chou The accreting millisecond pulsar XTE J1807-294 is studied through a pulse-shape modeling analysis. The model includes blackbody and Comptonized emission from the one visible hot spot and makes use of the Oblate Schwarzschild approximation ...
CONSTELLATION DELPHINUS, THE DOLPHIN
CONSTELLATION DELPHINUS, THE DOLPHIN

... 9.75 found by William Herschel September 24, 1785. At a distance of about 185,000 light-years, the globular cluster NGC 7006 is extremely remote. It is also fairly dim at magnitude 11.5. ...
Science Olympiad 2008 Reach for the Stars Division B
Science Olympiad 2008 Reach for the Stars Division B

... 70, 71. Of the planets visible today and tonight, are any of them in any of these 8 constellations? If so, list the planet and the constellation it is in. ...
Powerpoint - BU Imaging Science
Powerpoint - BU Imaging Science

... • Seems like that jovian planets DO form far from star in circular orbit – What happens after that? ...
Project 3. Colour in Astronomy
Project 3. Colour in Astronomy

... U=B=V=R=I=0 This does not mean that Vega show the same brightness through all filters. It is an arbitrary decision taken by the astronomers who have agreed on taking Vega as the zero point for the magnitude scale. Exercise 2: Spica and Antares are two well-known stars with colour indices (B-V)=0.13 ...
Read the information on Hertzsprung
Read the information on Hertzsprung

... In the Hertzsprung-Russell (HR) diagram, each star is represented by a dot. There are lots of stars out there, so there are lots of dots. The position of each dot on the diagram tells us two things about each star: its luminosity and its temperature. The vertical axis represents the star’s luminosit ...
Research Papers-Cosmology/Download/5936
Research Papers-Cosmology/Download/5936

... it assumed that star is rotating with a large number of revolutions n = 645 r/s. In this case, there is a danger that it will be broken by centrifugal forces. The force of gravity is opposes to the centrifugal forces. In order to prevent the destruction of stars, we have to assume that a radius of ...
The Night Sky September 2016 - Bridgend Astronomical Society
The Night Sky September 2016 - Bridgend Astronomical Society

... Andromedae - and move two stars to the left and up a bit. Then turn 90 degrees to the right, move up to one reasonably bright star and continue a similar distance in the same direction. You should easily spot M31 with binoculars and, if there is a dark sky, you can even see it with your unaided eye. ...
Celestial Distances - Wayne State University
Celestial Distances - Wayne State University

... Summary of Tools for Measuring Celestial Distances Within the solar system, distances are determined by timing how long it takes radar signals to travel from the Earth to a planet or other body and then return Distances to nearest stars can be measured using the parallax (triangulation) method For ...
The Life Cycle of Stars
The Life Cycle of Stars

... the formation of all the additional elements in the periodic table. Supernovas are rare astronomical events. One of the few supernovas that have been observed is the supernova that created the Crab Nebula in the year 1054 (Figure 8). Since the invention of the telescope 400 years ago, only one super ...
< 1 ... 34 35 36 37 38 39 40 41 42 ... 135 >

Star of Bethlehem



In Christian tradition, the Star of Bethlehem, also called the Christmas Star, revealed the birth of Jesus to the Biblical Magi, and later led them to Bethlehem. The star appears only in the nativity story of the Gospel of Matthew, where astrologers from the east are inspired by the star to travel to Jerusalem. There they meet King Herod of Judea, and ask where the king of the Jews had been born. Herod, following a verse from the Book of Micah interpreted as a prophecy, directs them to Bethlehem, to the south of Jerusalem. The star leads them to Jesus' home in the town, where they worship him and give him gifts. The wise men are then given a divine warning not to return to Herod so they return home by a different route.Many Christians see the star as a miraculous sign to mark the birth of the Christ (or messiah). Some theologians claimed that the star fulfilled a prophecy, known as the Star Prophecy. Astronomers have made several attempts to link the star to unusual astronomical events, such as a conjunction of Jupiter and Saturn, a comet or a supernova.Many modern scholars do not consider the story to be describing a historical event but a pious fiction created by the author of the Gospel of Matthew.The subject is a favorite at planetarium shows during the Christmas season, although the Biblical account describes Jesus with a broader Greek word, which can mean either ""infant"" or ""child"" (paidon), rather than the more specific word for infant (brephos), possibly implying that some time has passed since the birth. The visit is traditionally celebrated on Epiphany (January 6) in Western Christianity.
  • studyres.com © 2026
  • DMCA
  • Privacy
  • Terms
  • Report