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Spring Constellations
Spring Constellations

... means “ear of wheat.” Spica is a white star (hot), about 220 LY away, & 2000X the sun’s brightness. A whole group of galaxies is to the left of Leo’s tail & above Virgo’s head. The Sombrero Galaxy (M104) is due west of Spica. Virgo is usually associated with goddesses of fertility (Ishtar) & harvest ...
a transiting planet of a sun-like star
a transiting planet of a sun-like star

... transiting planets with periods between 3 and 4 days. Both the planetary radius and the inclination are functions of the spectroscopically determined stellar radius. If the stellar radius is 1:0  0:08 R, then the planetary radius is 1:30  0:11RJ and the inclination of the orbit is 87N7  1N2. We ...
What is an astrolabe
What is an astrolabe

stars - Moore Public Schools
stars - Moore Public Schools

... This mythological creature stood at the gates of the underworld and watched over this realm, as well as, the Osiris, the God of the Underworld. Every year, the Egyptians watched a celestial or sky drama unfold as the their God Horus, the son of Osiris, embarked on his journey to visit his father, c ...
Moon Search Algorithms for NASA`s Dawn
Moon Search Algorithms for NASA`s Dawn

... Nix and Hydra, that were discovered in 2005 [15-16]. These steps address various issues for satellite search due to motion, image misalignments, and artifacts. In this section, we demonstrate how one can resolve such barriers to satellite search by applying different computational approaches such as ...
Chemical composition of 90 F and G disk dwarfs
Chemical composition of 90 F and G disk dwarfs

... obtained for a sample of 90 F and G main-sequence disk stars covering the metallicity range −1.0 < [Fe/H] < +0.1, and have been analysed in a parallel way to the work of Edvardsson et al. (1993a) in order to re-inspect their results and to reveal new information on the chemical evolution of the Gala ...
Discovery of extremely lead-rich subdwarfs: does heavy metal signal
Discovery of extremely lead-rich subdwarfs: does heavy metal signal

... for each star are shown in Table 1 and also in Fig. 1. Errors given in Table 1 are formal errors from the χ 2 solution. y ≡ nHe /nH is also included. Since the measured values of Teff lie close to ≈40 000 K, the increasing importance of departures from local thermodynamic equilibrium (LTE) needs to ...
Galactic Evolution:
Galactic Evolution:

Foundations of Harappan Astronomy:
Foundations of Harappan Astronomy:

... 1) the evaporation in the southern hemisphere while it is winter in the north (around January in the present Epoch) 2) The movement of the moisture to the equatorial latitudes at Summer solstice (around March in the present epoch) 3) The amount of heating of the Indian subcontinental plate in early ...
Kepler and K2 Missions | NASA
Kepler and K2 Missions | NASA

... spacecraft following separation from the launch vehicle and for contingency safe mode pointing control. No propulsive capability for on-orbit delta-V is required since drift-away is constrained by control of launch vehicle dispersion errors. Uplink commanding and downlink real-time engineering data ...
Document
Document

... 9) Only use paddle control to slew the telescope to center the 2 stars Slewing speed is controlled from the numeric keypad (9 is the fastest, 1 is the slowest) ...
Using a distant X-ray source to detect small Transneptunian Objects
Using a distant X-ray source to detect small Transneptunian Objects

Chapter 20
Chapter 20

... • When fusion ceases in the core, it begins to collapse and heat. Hydrogen fusion starts in the shell surrounding the core. • The helium core begins to heat up; as long as the star is at least 0.25 solar masses, the helium will get hot enough that fusion (to carbon) will start. • As the core collaps ...
Stars - Emera Astronomy Center
Stars - Emera Astronomy Center

... 5-ESS1-1. Support an argument that differences in the apparent brightness of the sun compared to other stars is due to their relative distances from earth. 5-ESS1.A The Universe and its Stars. The sun is a star that appears larger and brighter than other stars because it is closer. Stars range great ...
Searching for the oldest, most metal-poor stars in the SkyMapper Survey
Searching for the oldest, most metal-poor stars in the SkyMapper Survey

... chemical evolution of the universe, which is the result of the nucleosynthesis of the elements within stars and supernova explosions. The most metal-poor stars are the oldest stars and thus provide information about the condition of the early universe. This research examined high-resolution spectra ...
PDF - Department of Statistics
PDF - Department of Statistics

ppt document - FacStaff Home Page for CBU
ppt document - FacStaff Home Page for CBU

... Way. By looking in the infrared (which is not scattered as much as visible light by the dust and gas), we see that we are not in the center of the disk, but somewhere away from the center. The approximate size of the Milky Way appears to be about 100,000 light years across and 2,000 light years thic ...
Parallax
Parallax

star - Cloudfront.net
star - Cloudfront.net

... 2. Although the stars that make up a pattern appear to be close together, they are not all the same distance from Earth. ...
The Mt John University Observatory search for Earth
The Mt John University Observatory search for Earth

... under construction for the ESO Very Large Telescope and G-CLEF (Szentgyorgyi et al. 2012) has been selected as a firstlight instrument for the Giant Magellan Telescope (GMT). However, there is an alternative to extreme precision: with a large enough number of measurements, even signals with amplitude ...
Created with Sketch. Satellite web hunt
Created with Sketch. Satellite web hunt

Astronomy Astrophysics
Astronomy Astrophysics

... determined. High resolution optical spectra of 22 stars obtained with the Keck I telescope are matched by synthetic spectra computed from a grid of NLTE model atmospheres. In this paper, the third in a series on white dwarf rotation, we concentrate preferentially on DA white dwarfs with convective a ...
The Atmospheric Instruments and Their Applications: GOMOS
The Atmospheric Instruments and Their Applications: GOMOS

Sample Exam for 3 rd Astro Exam
Sample Exam for 3 rd Astro Exam

... B. A UV photon that ionizes the gas around it. C. A radio photon of 21-cm wavelength that travels unimpeded through the galactic disk. D. A neutrino that passes through ordinary matter without effect. Which of the statements below best describes the spiral arms seen in some galaxies? A. Spiral arms ...
22 pm - Starmap
22 pm - Starmap

... The map shows what you see looking at the zenith. The apparent inversion of East and West compared to road maps is normal. Hold the map face down above your head, and the cardinal points will be oriented as usual. As a starting point, face North, holding the map in your eyesight direction, with its ...
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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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