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1. The catalogue structure
1. The catalogue structure

... of certain Almagest stars on the celestial sphere of our epoch suggested by said astronomers are also indicated. We have partially processed this enormous body of material. First of all, it is very useful to indicate the location of the constellations mentioned in Ptolemy’s star catalogue geometrica ...
Records of Ketu in stone inscriptions
Records of Ketu in stone inscriptions

... we need to explore other possibilities, for example a long period variable or explosive star. Our search yielded one possible candidate as NGC 7662, which is an extensively studied planetary nebula. Guerrero et al. 14 identified two ellipsoidal shells in this nebula and the kinematic ages were deriv ...
Condensates in Neutron Star Interiors
Condensates in Neutron Star Interiors

... On July 4th 1054, a supernova went off in the constellation of Taurus as observed widely by astronomers on Earth (and termed as nova stella, a new star). Centuries later, in 1731, John Bevis discovered the supernova remnant, which was later christened the Crab nebula (or M1, the first entry in the M ...
Notes - Bill Wolf
Notes - Bill Wolf

... brightness with a number scale. The first group of stars to become visible at night were called magnitude one, the next group to become visible were the magnitude two stars, and so on up to magnitude 6. It’s obvious here to note that stars with lower magnitude are actually the brighter stars. Later, ...
Science East Meteor Radiant Worksheet finished
Science East Meteor Radiant Worksheet finished

... unable to be traced back to a radiant is called a Sporadic and is not part of a meteor shower. These occur most nights of the year. Comet: A comet is a body that orbits around the sun. The nucleus of the comet is composed of rock, dust and ice. The tail of the comet is caused by solar radiation vapo ...
Thu th surf c
Thu th surf c

... The velocity curve shows the radial velocity changes due to pulsation alone, and since the star itself is moving toward the sun with a velocity of - 10 miles per second, its radial velocity relative to the sun is also given. ...
LET THE STARS GET IN YOUR EYES SKY MOTIONS
LET THE STARS GET IN YOUR EYES SKY MOTIONS

... One of the first steps in sky watching is learning to recognize constellations. Learning constellations requires a constellation chart, a red flashlight and your willingness to explore the sky. A red flashlight is a basic tool of astronomers because it won't ruin your night vision. You can paint you ...
Chapters 12 and 13 Review: The Life Cycle and Death of Stars
Chapters 12 and 13 Review: The Life Cycle and Death of Stars

Is the central binary system of the planetary nebula Henize 2
Is the central binary system of the planetary nebula Henize 2

Angle d = Latitude Angle c = Altitude Polaris Angle c
Angle d = Latitude Angle c = Altitude Polaris Angle c

... celestial equator to the zenith > latitude, say 50 deg, then Alt = 90 + (Phi + Dec) rather than (90 – Phi) + Dec Alt = 90 + Our Observing Latitude determines what celestial objects are seen above our local horizon ...
Here - Astrophysics Research Institute
Here - Astrophysics Research Institute

... • Celestial Meridian – a great circle which passes through Zenith and the North & South celestial poles. It is perpendicular to the horizon. If you stand facing North, the meridian is a line that passes from north on the horizon, directly over your head, to south on the horizon behind you ...
Aldebaran
Aldebaran

... condense further and heat up. Nuclear reactions occurred when the temperature in the center of the protostar reached about 10 million degrees, and the star was born. Further expansion and heating of the star’s exterior then led to the formation of a red giant. This is what Aldebaran is now. Aldebara ...
A dust ring around Epsilon Eridani: analogue to the young Solar
A dust ring around Epsilon Eridani: analogue to the young Solar

... Earth-like planets occur frequently, then life may exist elsewhere in our Galaxy. However, the search for extra-terrestrial planetary systems is extremely difficult, and is most often approached indirectly. Massive planets introduce changes in the observed velocities of their stars (the Doppler tech ...
The Antares Emission Nebula and Mass Loss of α Sco A
The Antares Emission Nebula and Mass Loss of α Sco A

... that faint [Fe II] emission is seen all along the slit, i.e. in the neutral M star wind. The explanation comes from the observation that one of the allowed lines, Fe II 5169 Å, appears both in the neutral wind (position 0.9 from the M star) and in the H II region. Apparently one channel for the exc ...
November, 2015 - The Baton Rouge Astronomical Society
November, 2015 - The Baton Rouge Astronomical Society

... 847 and counting: that’s the number of planets confirmed as existing around 642 stars within several hundred light-years of our Sun. And more than 2,000 additional detections are awaiting confirmation by follow-up observations. By far, the most potential exoplanets have been found by the NASA spacec ...
Chapter 30: Stars
Chapter 30: Stars

Document
Document

... • Bright (V ~ 21 at 110 kpc) • Variable stars (P ~ 0.6 day) with distinct light curves ( ~1 mag amplitude) → easily identifiable ...
The plane of the Moon`s orbit has an inclination of 5.15 degree to
The plane of the Moon`s orbit has an inclination of 5.15 degree to

... which were seen within a group of other stars surrounding each of them in a recognizable form or shape in the sky. Krittika nakshatra is also recognized by the star Krittika (Aclyone 2) whose longitude is about 360 8'. The value of the Lahiri ayanamsa was 230 53' 56”.3 on 1.1. 2003. Thus the present ...
Introduction: The History and Technique of Stellar Classification
Introduction: The History and Technique of Stellar Classification

... Introduction: The History and Technique of Stellar Classification Patterns of absorption lines were first observed in the spectrum of the sun by the German physicist Joseph von Fraunhofer early in the 1800’s, but it was not until late in that century that astronomers were able to routinely examine t ...
September - Rose City Astronomers
September - Rose City Astronomers

... of Japan’s leading makers of fine telescopes, the #339 was distributed worldwide. Many thousands of units were sold over a twenty-year time period. The 600 power telescope, due to its popularity, was remarketed by a number of different companies with their own model numbers. Meade ran continual ads ...
Calculating Parallax Lab
Calculating Parallax Lab

... Even when observed with the largest telescopes, stars are still just points of light. Although we may be able to tell a lot about a star through its light, these observations do not give us a reference scale to use to measure their distances. We need to rely on a method that you are actually already ...
Alpha Centauri
Alpha Centauri

... Alpha Centauri Was often called Rigel Kentaurus.  Rigel Kentaurus means “foot of the centaur” in Arabic. ...
A very massive runaway star from Cygnus OB2⋆
A very massive runaway star from Cygnus OB2⋆

... v∗ is the spatial velocity of the star. The distance given in Eq. (5) assumes that the bow shock is bound by shock fronts on both sides. In reality, the non-zero cooling time of the shocked stellar wind builds up a thick layer of low-density, high-temperature gas between the reverse shock on the ste ...
USRA - MSU Solar Physics
USRA - MSU Solar Physics

... the 10-m telescope in Hawaii which reveled that its redshift was at least 0.835. In other words, it was more than 6 billion lightyears away! Every question answered adds at least ten more questions unsolved. Even though the distance riddle has been solved, many more questions remain. Two prevailing ...
15_Testbank
15_Testbank

... D) Because there is still uncertainty over what generates the energy in stellar cores. E) Because it refers to stellar masses and these were difficult to measure accurately. Answer: B 16) Which of the following statements about spectral types of stars is true? A) The spectral type of a star can be u ...
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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.
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