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Astronomy Timeline This is a timeline of important events
Astronomy Timeline This is a timeline of important events

... TeideAstro - educación ambiental ...
Summer - Dark Sky Discovery
Summer - Dark Sky Discovery

... lucky, and get a very dark night, you might be able to see the Milky Way, our galaxy, down which Cygnus appears to fly. The other star on the southern chart is Arcturus. If you follow the curve of the handle of the Plough, you will eventually arrive at Arcturus. This is sometimes called the ‘arc to ...
On the nature of early-type emission line objects in NGC6611
On the nature of early-type emission line objects in NGC6611

Chapter 24
Chapter 24

... Properties of stars Distance • Measuring a star's distance can be very difficult • Stellar parallax • Used for measuring distance to a star • Apparent shift in a star's position due to the orbital motion of Earth • Measured as an angle • Near stars have the largest parallax • Largest parallax is l ...
Starlight and What it Tells Us
Starlight and What it Tells Us

... • Color is directly related to temperature • Temperature is the only determinant of color • Energy per unit area is the same if temperature is the same – If two stars have the same color and distance, difference in brightness is due to difference in size – Dwarf and giant stars are literally dwarfs ...
Chapter2
Chapter2

... on Earth’s Climate Factors affecting Earth’s climate: • Eccentricity of Earth’s orbit around the Sun (varies over period of ~ 100,000 years) • Precession (Period of ~ 26,000 years) ...
J tieutifit meti(au.
J tieutifit meti(au.

... naked eye, on a clear night, detects a hazy speck. It 15th, the first quarter on the 22d, full moon on the machinery required by the operation of the street is the Great Nebula of Andromeda, and its central 29th, and last quarter on the 7th. The moon is near­ cable system. l!"'or a time the cable ap ...
Search for Student Research Assistant
Search for Student Research Assistant

... (other than the Sun). Of the two stars, one is a normal star, slightly less massive than our own Sun, but the other is a neutron star (a collapsed star only about 10 km across). Sco X-1 was the first discovered star system of its type. It is particularly interesting because although it has a neutron ...
Exoplanets Properties of the host stars Characterization of the
Exoplanets Properties of the host stars Characterization of the

... –  A good knowledge of the properties of the stars hosting exoplanets is fundamental to improve the accuracy of exoplanet measurements –  Accurate determination of stellar masses and radii are required to derive masses and radii of the planets detected with the Doppler and transit methods, respectiv ...
star
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... stars can be seen with a telescope, but the presence of the companion star is revealed by spectroscopy Such stars are called spectroscopic binaries The binary nature is indicated in the periodic Doppler-shift of their spectral lines as they orbit around each other Animation ...
Volcanoes and Igneous Activity Earth
Volcanoes and Igneous Activity Earth

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A Star is a ball of matter that is pulled together by gravity, and that
A Star is a ball of matter that is pulled together by gravity, and that

... How bright a star is when viewed from___________. A very large, hot star could look dim just because it is so far away. •_____________________Magnitude: the amount of ____________ that is actually given off by a star. 4. Measuring the Distance to Stars: we measure the distance between objects in spa ...
Parallax and Its role In the helIocentrIc/GeocentrIc debate
Parallax and Its role In the helIocentrIc/GeocentrIc debate

Astronomical Distance Determination • etc.
Astronomical Distance Determination • etc.

... seen from far away. (They are not main sequence stars). A complication though is that there are two populations of Cepheids and they have different period luminosity ...
Lecture 10 Spectra of Stars and Binaries
Lecture 10 Spectra of Stars and Binaries

... •  Leader
of
Pickering’s
“computers”,
she
noZced
 subtle
paJerns
among
metal
lines.
 •  Re‐arranged
Pickering’s
ABC
spectral
types,
 throwing
out
most
as
redundant.
 •  Lef
7
primary
and
3
secondary
classes:
 •  O

B

A

F

G

K

M

(R

N

S)
 ...
Guide to Deep Space Poster PDF
Guide to Deep Space Poster PDF

... Light travels as a wave, and hence it has a wavelength. If you imagine waves in the ocean, their wavelength is the distance between each crest. Just for a moment think about the familiar colours of the rainbow (or spectrum). At one side we start with red which has a long wavelength, next orange with ...
2. Stellar Physics
2. Stellar Physics

... fusion reactions in the stellar interior Other energy sources are dominant during star formation and stellar death: • Star formation - before the interior is hot enough for significant fusion, gravitational potential energy is radiated as the radius of the forming star contracts. Protostellar or pre ...
September 2012 night sky chart
September 2012 night sky chart

... The spring equinox occurs on the 23rd when the length of day and night is almost equal, about 12 hours each. Saturn is visible low in the west in the constellation of Virgo. Mars is next to the star Zubenelgenubi in Libra. The best time to see the Moon using binoculars or a small telescope is a few ...
Standard EPS Shell Presentation
Standard EPS Shell Presentation

... Parallax is the apparent change in position of an object when you look at it from different directions. ...
Measuring the Sky - Physics and Astronomy and more!
Measuring the Sky - Physics and Astronomy and more!

... Read Airy’s pamphlet on the Uranus problem 1841:"Formed a design in the beginning of this week, of investigating, as soon as possible after taking my degree, the irregularities of the motion of Uranus, which are yet unaccounted for; in order to find out whether they may be attributed to the action o ...
Life of stars, formation of elements
Life of stars, formation of elements

... • Built up of molecules of most common elements after hydrogen and helium • Core: Silicates or Graphite (Si, O, C) • Mantle: C,N,O combined with H ...
Problem Sheet for Introduction to Astrophysics
Problem Sheet for Introduction to Astrophysics

... a) If you could stand on the event horizon of a one-solar-mass black hole (M=1.991030 kg), what is the tidal force acting on you? (Assume your weight is 70kg and your height is 2 m) b) If you could stand on the event horizon of a 109 solar mass black hole, what is the tidal force acting on you (the ...
Lucas - WordPress.com
Lucas - WordPress.com

... The Double­Double (ε Lyrae) looks like two stars in binoculars, but a good telescope shows that both of these two are themselves binaries. However, there may be as many as ten stars in this system! The distant pairs are about 0.16 light­year apart and take about half a million years to orbit one ano ...
Laboratory Procedure (Word Format)
Laboratory Procedure (Word Format)

... without first organizing their information about the vast number of stars in some systematic system. The geometric arrangement of some stars provided the Greeks with a natural organizational system which we call constellations. By connecting the stars with imaginary lines, the ancients saw pictures ...
Review 3 - Physics and Astronomy
Review 3 - Physics and Astronomy

... 2. Detecting parallaxes means that Earth orbits around Sun 3. Maximum parallactic shift (two positions of the Earth’s orbit 6 months apart) ...
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Hipparcos



Hipparcos was a scientific satellite of the European Space Agency (ESA), launched in 1989 and operated until 1993. It was the first space experiment devoted to precision astrometry, the accurate measurement of the positions of celestial objects on the sky. This permitted the accurate determination of proper motions and parallaxes of stars, allowing a determination of their distance and tangential velocity. When combined with radial-velocity measurements from spectroscopy, this pinpointed all six quantities needed to determine the motion of stars. The resulting Hipparcos Catalogue, a high-precision catalogue of more than 118,200 stars, was published in 1997. The lower-precision Tycho Catalogue of more than a million stars was published at the same time, while the enhanced Tycho-2 Catalogue of 2.5 million stars was published in 2000. Hipparcos‍ '​ follow-up mission, Gaia, was launched in 2013.The word ""Hipparcos"" is an acronym for High precision parallax collecting satellite and also a reference to the ancient Greek astronomer Hipparchus of Nicaea, who is noted for applications of trigonometry to astronomy and his discovery of the precession of the equinoxes.
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