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The ultra-luminous x-ray sources near center of M82
The ultra-luminous x-ray sources near center of M82

...  Chandra 0.3-7 keV images of the central 45”45” region of M82 1999-09-20 ObsID 361 ...
the magellanic clouds newsletter - Keele University Astrophysics
the magellanic clouds newsletter - Keele University Astrophysics

... Symbiotic stars are long-orbital-period interacting-binaries characterized by extended emission over the whole electromagnetic range and by complex photometric and spectroscopic variability. In this paper, the first of a series, we present OGLE light curves of all the confirmed symbiotic stars in th ...
Andromeda Nebula Lies Outside Milky Way Galaxy
Andromeda Nebula Lies Outside Milky Way Galaxy

... "Red Shift" is Proof of Einstein's General Theory Using the 100-inch Hooker Telescope at Mount Wilson Observatory, Dr. Edwin Hubble has studied many spiral nebulae. He has discovered they are moving away from us at a rapid pace. This is strong evidence of an expanding universe. He has further determ ...
Habitable planets around the star Gliese 581?
Habitable planets around the star Gliese 581?

... derive theoretical and empirical habitable distances for stars of F, G, K, and M spectral types. Results. Planets Gl 581c and Gl 581d are near to, but outside, what can be considered as the conservative habitable zone. Planet “c” receives 30% more energy from its star than Venus from the Sun, with a ...
Chapter 13 Other Planetary Systems: The New Science of Distant
Chapter 13 Other Planetary Systems: The New Science of Distant

... It has a planet orbiting at less than 1 AU. It has a planet orbiting at greater than 1 AU. It has a planet orbiting at exactly 1 AU. It has a planet, but we do not have enough ...
Lec2015_22
Lec2015_22

... stellar content of the disk of our Galaxy, with ages <9Gyr (white dwarf age for Galactic Disk – Lecture 19) • The Halo of our Galaxy is made up predominantly of Population II stars that also have some evidence for enrichment from massive stars, although many of the stars possess only 1/100th of the ...
The star and the colours
The star and the colours

... Narrator 1: And from her mouth a big rainbow comes out: Narrator 2: Red, orange, yellow Narrator 3: Green, blue, purple and violet! Star: ...
1 Introduction - University of Amsterdam
1 Introduction - University of Amsterdam

I. Early History of Astronomy
I. Early History of Astronomy

ADAS Simple Guide to Telescope Instrumentation and Operation
ADAS Simple Guide to Telescope Instrumentation and Operation

... The Setting Circles consist of two graduated disks attached to the right ascension (RA) and declination (DEC) axis of an equatorial mount as illustrated above. The right ascension disk is graduated into hours, minutes, and seconds. The declination disk is graduated into degrees, minutes, and seconds ...
The loss of nitrogen-rich atmospheres from Earth-like
The loss of nitrogen-rich atmospheres from Earth-like

... gaseous envelope even if the planet orbits its parent M star within the habitable zone (HZ). However, as shown in Lammer et al. (2007), a high CO2 atmospheric mixing ratio will result in enhanced IR cooling in the thermosphere and inhibits its expansion and therefore leads to reduced non-thermal atm ...
Journey through the cosmos
Journey through the cosmos

... It is called the Milky Way because it looks like a giant splash or river of milk across a dark sky. But you probably haven’t seen it look like this, unless you live somewhere a long way away from a town. Until 150 years ago, the Milky Way was the most obvious thing in the night sky. Light pollution ...
Chapter 2: The Copernican Revolution
Chapter 2: The Copernican Revolution

... to dispense with the epicycles for Mercury, Venus, Mars, Jupiter and Saturn.  How then does Copernicus  explain the retrograde motions of these planets?  From a Copernican perspective, the retrograde motions of the planets are an illusion, caused by the  earth’s own motion.  Suppose you’re driving  ...
The Quest for Object X - Department of Physics and Astronomy
The Quest for Object X - Department of Physics and Astronomy

... Does the object move? Most objects outside of our solar system show such small motions that they appear stationary, except over periods of thousands or millions of years. But objects in the solar system, since they are in orbit around the sun, appear to move relatively quickly among the stars. The m ...
the search for object x
the search for object x

... Does the object move? Most objects outside of our solar system show such small motions that they appear stationary, except over periods of thousands or millions of years. But objects in the solar system, since they are in orbit around the sun, appear to move relatively quickly among the stars. The m ...
STApr18
STApr18

OBJXlab
OBJXlab

... Does the object move? Most objects outside of our solar system show such small motions that they appear stationary, except over periods of thousands or millions of years. But objects in the solar system, since they are in orbit around the sun, appear to move relatively quickly among the stars. The m ...
Goal: To understand what comets are and to explore the Oort cloud.
Goal: To understand what comets are and to explore the Oort cloud.

... millions of years) come from the Oort cloud. • Oort cloud objects probably formed in the gas giant region and were probably tossed there by Jupiter. • They are usually a bit bigger than short period comets, and higher densities. • A bright one comes into the inner solar system every 5-10 years. • Te ...
doc - Steve Kluge
doc - Steve Kluge

... 3. On what day (approximately) will Venus pass between the Earth and the Sun?______________. Venus passes across the Sun (transits the Sun) once every 1.6 years, yet the Sun is never eclipsed by Venus. Why don’t transits of Venus produce eclipses on earth? _________ _________________________________ ...
September 2016
September 2016

... of the triplet to us and the closest known star to us. ...
the orbit of venus
the orbit of venus

... 3. On what day (approximately) will Venus pass between the Earth and the Sun?______________. Venus passes across the Sun (transits the Sun) once every 1.6 years, yet the Sun is never eclipsed by Venus. Why don’t transits of Venus produce eclipses on earth?___________________ ________________________ ...
The extreme ultraviolet and X-ray Sun in Time: High
The extreme ultraviolet and X-ray Sun in Time: High

... of four young clusters with ages of ∼150 Myr and used a rotational evolution model to predict the evolution of the resulting distribution of Ω on the MS. The sample contains 1556 stars in the 0.4−1.1 M mass range. In Fig. 1, we show predictions for the distributions of LX based on these Ω distribut ...
Planets
Planets

The Milky Way Galaxy
The Milky Way Galaxy

... Radar ranging - good for measuring distances in the solar system (up to about 0.0001 light years) Parallax - good for measuring distances to a few hundred light years ...
ART. VULCAN/05
ART. VULCAN/05

... begins 3 to 4 days before the earthquake itself, sometimes 5 days, to one week before. A kind of energetic gap inbetween those days of «preparation» is also observed – usually one to two days before the event – that needs to be carefully analysed and coupled to the study of the daily path of the Moo ...
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Aquarius (constellation)



Aquarius is a constellation of the zodiac, situated between Capricornus and Pisces. Its name is Latin for ""water-carrier"" or ""cup-carrier"", and its symbol is 20px (Unicode ♒), a representation of water.Aquarius is one of the oldest of the recognized constellations along the zodiac (the sun's apparent path). It was one of the 48 constellations listed by the 2nd century AD astronomer Ptolemy, and it remains one of the 88 modern constellations. It is found in a region often called the Sea due to its profusion of constellations with watery associations such as Cetus the whale, Pisces the fish, and Eridanus the river.
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