Factbites
 Where results make sense
About us   |   Why use us?   |   Reviews   |   PR   |   Contact us  

Topic: Wilhelm Gliese


In the News (Thu 31 Dec 09)

  
  Wilhelm Gliese -- Facts, Info, and Encyclopedia article   (Site not responding. Last check: 2007-10-08)
Wilhelm Gliese (June 21 1915 – June 12 1993) was a German astronomer.
He worked at the Astronomisches Rechen-Institut, first in (Capital of Germany located in eastern Germany) Berlin and then in (additional info and facts about Heidelberg) Heidelberg.
He is best known for his Gliese Catalogue of Nearby Stars, and some stars are best known by the catalogue number he gave them, such as (additional info and facts about Gliese 710) Gliese 710.
www.absoluteastronomy.com /encyclopedia/w/wi/wilhelm_gliese.htm   (82 words)

  
 Gliese 229 - Wikipedia, the free encyclopedia
A simulated image of Gliese 229 from a distance of 2,081,000 km (1,293,000 miles).
Gliese 229 is a cool, red star, and is a companion to Gliese 229b, a brown dwarf - a failed star.
Gliese 229b is thought to be 20 to 50 times the mass of Jupiter, thus too large to be classified a planet, but too small to ignite and become a star.
en.wikipedia.org /wiki/Gliese_229   (109 words)

  
 Gliese 710
Many astronomers now refer to this star as Gliese 710 by its designation in the famous Gliese Catalogue of Nearby Stars (CNS, now ARICNS database) of Wilhelm Gliese (1915-93), who was a longtime astronomer at the Astronomiches Rechen-Institut at Heidelberg (even when it was at Berlin).
Gliese 710 is a relatively dim, main sequence orange-red or red dwarf star of spectral and luminosity K5-M1 V (ARICNS; Joy and Abt, 1974; and Upgren et al, 1972).
Gliese 710 B? According to García-Sánchez et al (1999), astrometric residuals in early proper-motion measurements suggested a possible periodicity of 4.7 years (around 1,700 days) but its significance was uncertain (Grossenbacher et al, 1968; and V.
www.solstation.com /stars2/gl710.htm   (978 words)

  
 Gliese 876 -- Facts, Info, and Encyclopedia article   (Site not responding. Last check: 2007-10-08)
Gliese 876 c is a (Any of the four outermost planets in the solar system; much larger than Earth and gaseous in nature (like Jupiter)) gas giant half the size of ((Roman mythology) supreme god of Romans; counterpart of Greek Zeus) Jupiter, discovered in 2001.
This means that the planet itself would be partly made up of water (A visible mass of water or ice particles suspended at a considerable altitude) clouds.
Gliese 876 b is a gas giant twice the size of Jupiter.
www.absoluteastronomy.com /encyclopedia/G/Gl/Gliese_876.htm   (173 words)

  
 Gliese 86 / HR 637 AB
Many astronomers now refer to this star by its designation in the famous Gliese Catalogue of Nearby Stars (CNS, now ARICNS database) of Wilhelm Gliese (1915-93), who was a longtime astronomer at the Astronomiches Rechen-Institut at Heidelberg (even when it was at Berlin).
Gliese 86 is an orange-red main-sequence dwarf star of spectral and luminosity type K0-1 V. The star may have 79 percent of Sol's mass (Observatoire de Genève), 86 percent of its diameter (Johnson and Wright, 1983, page 649), and 35 percent of its luminosity.
Gliese 229 b with satellite as imagined by Whatmough.
members.nova.org /~sol/solcom/stars2/gl86.htm   (1285 words)

  
 Gliese 876 / Ross 780
However, many astronomers now refer to this star by its designation in the famous Gliese Catalogue of Nearby Stars (CNS, now ARICNS database) of Wilhelm Gliese (1915-93), who was a longtime astronomer at the Astronomiches Rechen-Institut at Heidelberg (even when it was at Berlin).
A preliminary analysis by Jeffrey A. Valenti in 1998 of the spectrum of the star suggested that the star is less enriched than Sol in elements heavier than hydrogen ("metal-poor") by a factor of two to three, but one team of astronomers apparently now believes that it may be as enriched as Sol (exoplanets.org).
Gliese 876 is a variable star with the designation "IL Aquarii." Some other useful star catalogue designations include: IL Aqr, Gl 876, Hip 113020, BD-15 6290, G 156-57, LHS 530, LTT 9244, LPM 841, LFT 1745, Vys 337, and Ross 780.
www.solstation.com /stars/gl876.htm   (1742 words)

  
 Wilhelm Gliese - Wikipedia, the free encyclopedia
Wilhelm Gliese (June 21, 1915 – June 12, 1993) was a German astronomer.
He is best known for his Gliese Catalogue of Nearby Stars, and some stars are best known by the catalogue number he gave them, such as Gliese 710.
This page was last modified 19:27, 18 October 2005.
en.wikipedia.org /wiki/Wilhelm_Gliese   (80 words)

  
 Super-Earth Sought and Found :: Astrobiology Magazine :: Search for Life in the Universe
Gliese 876 (or GJ 876) is a small, red star known as an M dwarf the most common type of star in the galaxy.
Lissauer and Rivera have been analyzing Keck data on the Gliese 876 system in order to model the unusual motions of the two known planets, and three years ago got an inkling that there might be a smaller, third planet orbiting the star.
The team plans to continue to observe the star Gliese 876, but is eager to find other terrestrial planets among the 150 or more M dwarf planets they observe regularly with Keck.
www.astrobio.net /news/modules.php?op=modload&name=News&file=article&sid=1601   (1609 words)

  
 CNS3 - Gliese Catalog of Nearby Stars, 3rd Edition
The original catalogue and the notes describing it were prepared by Wilhelm Gliese and Hartmut Jahreiss, Astronomisches Rechen-Institut, Moenchhofstrasse 12-14, D-6900 Heidelberg 1, Germany, in 1991.
All new nearby stars have not yet been given Gliese (Gl) or Gliese and Jahreiss (GJ) numbers and those stars were all given the name of "NN" in the original version of this catalogue.
Generally, the preferred designations are GL, e.g., GL 10, the Gliese number, or the designation given to the star in the 2nd version of the Gliese Catalog (Gliese 1969), or GJ, e.g., GJ 1001, also often called the Gliese number, and derived from a tabulation of Gliese and Jahreiss (1979, Astr.
heasarc.gsfc.nasa.gov /W3Browse/star-catalog/cns3.html   (1253 words)

  
 FLICKER ALLEY - PHANTOM
Friedrich Wilhelm Murnau was born as Friedrich Wilhelm Plumpe on December 28th, 1888 in Bielefeld, Germany.
Friedrich Wilhelm Murnau's first films were also characterized by exotic subjects and crime stories.
Friedrich Wilhelm Murnau was buried on April 13th, 1931 in the Waldfriedhof Stahnsdorf, a cemetery at the outskirts of Berlin.
www.flickeralley.com /fa_phantom_03.html   (1610 words)

  
 [No title]
Three stars (Gliese 59, 67 and 68) are known as Old Population I and are almost certainly younger than the sun.
Because Gliese 86 has a velocity, eccentricity and inclination similar to 82 Eridani, it seems likely that its chemical composition may also not have severe metal deficiencies, but be similar to those of 82 Eridani.
Gliese 67 is a young star of at least solar metal abundances, considering its low velocity and eccentricity.
www.anomalies.net /ufo/ufodocs/text.documents/z/zetareti.ufo   (15354 words)

  
 Milky Way: Structure   (Site not responding. Last check: 2007-10-08)
From Gliese's catalog, which contains 1,049 stars in a volume with a radius of 65 light-years, the average calculated density is less than one-third the calculated density for stars within 17 light-years.
Gliese has estimated that when incompleteness of the catalogs is taken into account, the true stellar density is on the order of 0.004 stars per cubic light-year, which includes the probable number of unseen companions of multiple systems.
The density distribution of stars can be combined with the luminosity-mass relationship to obtain the mass density in the solar neighbourhood, which includes only stars and not interstellar material.
www.space.com /reference/brit/milkyway/structure.html   (6025 words)

  
 The Zeta Reticuli Incident
The Gliese catalog uses photometric, trigonometric and spectroscopic parallaxes and derives a mean from all three after giving various mathematical weights to each value.
Marjorie Fish was aware of the catalog variations, but has assumed the Gliese catalog is the most reliable source material to utilize.
One significant fact against a charade is that the data from the Gliese catalog was not published until 1969, five years after the star map was drawn by Betty Hill.
www.astrosurf.com /lunascan/hillzeta.htm   (6679 words)

  
 The world's top star catalogue websites
The Gliese (later Gliese-Jahreiss) catalogue attempts to list all stars within 20 parsecs of Earth (later editions expanded the coverage to 25 parsecs).
Although this version of the catalogue was termed "preliminary", it is still the current one as of September 2001, and is referred to as CNS3.
Unlike the Gliese, it does not cut off at a given distance from the Sun; rather it attempts to catalogue all known measured parallaxes.
dirs.org /wiki-article-tab.cfm/star_catalogue   (1787 words)

  
 glbtq >> arts >> Murnau, Friedrich Wilhelm
Working with many of his colleagues from Germany, including scenarist Carl Mayer, cameraman Karl Struss, and art director Rochus Gliese, this "song of two humans" remains one of the most beautiful films ever made, a magical parable about a peasant couple whose love is threatened but who find renewed commitment.
An imposingly tall, thin man of artistocratic demeanor, Murnau (born Friedrich Wilhelm Plumpe on December 28, 1888 in Bielefeld, Germany) was the product of the artistic ferment of the Weimar Republic.
Before embarking on his career as a filmmaker, he trained as an art historian, which may explain the painterly images of his films and the primacy he accorded to the visual.
www.glbtq.com /arts/murnau_fw.html   (942 words)

  
 Ancient Suns — FAQ: Gliese
Also known as the Catalog of Nearby Stars, the Gliese Catalog was the first concerted effort to list all of the stars near our own.
Three editions have been compiled by the German astronomer, Wilhelm Gliese, for which the catalog was named.
By 1991, when the preliminary version of the third edition came out, the number of stars known to exist within 25 parsecs had swelled to nearly 4,000.
ancientsuns.com /faq/gliese.html   (138 words)

  
 The Zeta Reticuli Incident
A suspicious alignment, detected in late 1968, turned out to be almost a perfect match once new data from the detailed 1969 edition of the Catalog of Nearby Stars became available (this catalog is often called the “Gliese catalog” -- pronounced “glee-see” -- after its principal author, Wilhelm Gliese).
The data on some of the stars in the map is just not good enough to make a definitive statement (the fact that measurements of most of the stars in question can only be made at the relatively poor equipped southern hemisphere observatories accounts for the less reliable data).
The scientific director of the U.S. Naval Observatory, K.A. Strand, is among the world’s foremost authorities on stellar distances for nearby stars.
www.bibliotecapleyades.net /vida_alien/zetareticuli_incident01.htm   (6072 words)

  
 NStars1CNS: Nearby star catalogues and PMSU   (Site not responding. Last check: 2007-10-08)
Probably the primary exponent of this approach to constructing a local census was Wilhelm Gliese.
Extending the distance limit to 22 parsecs (parallaxes exceeding 44 mas), Gliese increased the sample size to 1890 stars in 1529 systems, and data for those stars were published in 1969 as the Catalogue of Nearby Stars (Gliese, 1969: CNS2).
Data continued to accumulate during the 80s, and Gliese and Jahreiss continued to compile those results, producing an electronic version of a third version of the catalogue in the early 90s (Jahreiss & Gliese, 1991, pCNS3).
dept.physics.upenn.edu /~inr/pmsu.html   (3861 words)

  
 Elusive Earths :: Astrobiology Magazine :: Search for Life in the Universe
In this interview with Astrobiology Magazine, Professor of Astronomy Geoff Marcy, one of the world's leading planet-hunters, reflects on recent other-worldly discoveries and speculates on what surprises may lay in store.
View of Gliese 876 and a ringed Jupiter-class planet from an icy moon.
They orbit 55 Cancri, HD 190360, and Gliese 436.
www.astrobio.net /news/modules.php?op=modload&name=News&file=article&sid=1611   (1905 words)

  
 How small are small stars really?
It was discovered in 1894 by a Scottish astronomer, Robert Thorburn Ayton Innes (1861 - 1915), during a stay at the Cape Observatory (South Africa), due to its very fast motion on the sky, about 3.9 arcsec/year.
It is also designated GJ 551, the 551st entry in the "Catalogue of Nearby Stars", published in 1969 by two German astronomers, Wilhelm Gliese (1915-93) and Helmut Jahreis.
The visual magnitude is 11, or 100 times fainter than what can be perceived with the unaided eye on a dark sky; the parallax measured by the ESA Hipparcos astrometric satellite is 772.33 +- 2.42 milliarcsec, corresponding to a distance of 4.22 light-years.
www.eurekalert.org /pub_releases/2002-11/eso-hsa112902.php   (1430 words)

  
 UFO Area The Zeta Reticuli Incident   (Site not responding. Last check: 2007-10-08)
This table lists all known stars within a radius of 54 light-years that are single or part of a wide multiple star system.
Data is from the Gliese Catalog of Nearby Stars (1969 edition).
(This pair -- Gliese 201 and Gliese 202, a K5e and F8Ve pair separated by 0.15 light-years -- is currently being investigated.) Zeta Reticuli is indeed a rare case.
www.ufoarea.com /abduction_zeta.html   (15696 words)

  
 BD-05 1844 / Gl 250 AB
Many astronomers now refer to this star system by its designation in the famous Gliese Catalogue of Nearby Stars (CNS, now ARICNS database) of Wilhelm Gliese (1915-93), who was a longtime astronomer at the Astronomiches Rechen-Institut at Heidelberg (even when it was at Berlin).
The system's designation of BD-05 1844 comes from a catalogue that was originally published in 1863 by Friedrich Wilhelm August Argelander (1799-1875) on the position and brightness of 324,198 stars between +90° and -2° declination that were measured over 11 years from Bonn, Germany with his assistants Eduard Schönfeld (1828-1891) and Aldalbert Krüger (1832-1896).
For Star B, the water zone orbit lies near 0.076 AU.
members.nova.org /~sol/solcom/stars/gl250ab.htm   (746 words)

  
 Paul Wegener page in Classic Horror Players Directory
The film, co-directed by Wegener with Rochus Gliese, is about an Indian mystic uses his power of invisibility to scare a young inventor.
The film, co-written and co-directed by Wegener with Rochus Gliese, is about a monstrous Wild Man of folklore who threatens a village with destruction until he is pacified by the love of an understanding woman.
With Lyda Salmonova, Wilhelm Diegelmann, Fritz Feld (the pageboy), Rochus Gliese, Emilie Kurz, Erich Schönfelder and Friedrich Veilchenfeld.
myweb.wvnet.edu /~u0e53/paulwegener.html   (1302 words)

  
 [No title]   (Site not responding. Last check: 2007-10-08)
Preliminary Version of the Third Catalogue of Nearby Stars Wilhelm Gliese and Hartmut Jahreiss Astronomisches Rechen-Institut Heidelberg, Germany The present version of the CNS3 contains all known stars within 25 parsecs of the Sun.
It depends mainly on a preliminary version (Spring 1989) of the new General Catalogue of Trigonometric Parallaxes (YPC) prepared by Dr. William F. van Altena (Yale University).
22 (1969) GJ Gliese & Jahreiss, A&AS, 38, 423 (1979) Wo Woolley et al., Roy.
www.maa.agleia.de /Cat/Vol1/Nearbyst/cns3.doc   (388 words)

  
 THE ZETA RETICULI INCIDENT
eccentricities are 82 Eridani (Gliese 139) and Gliese 86.
Gliese 67 is a young star of at least solar metal
Gliese 86 and two others from a set of five candidates.
www.think-aboutit.com /aliens/THEZETARETICULIINCIDENT.htm   (12429 words)

  
 ch2.10
In the special case of nearby M dwarf stars, it may even be possible to detect large terrestrial planets.
In the Gliese catalog there are 248 star systems with binary separations between 0.2 and 15.0 arcsec.
Almost all of these stars are main-sequence (luminosity class V), but 16 are subgiants (luminosity class IV) and 2 are giants (luminosity class III).
history.nasa.gov /CP-2156/ch2.10.htm   (3990 words)

  
 UFO Archive Document: The Zeta Reticuli Incident By Terence Dickinson
Gliese 75 28.6 5.6 0.4 K0 Beta Canum
Gliese 86 37 6.1 0.4 K0 Mu Arae 37 5.1 0.9 G5 Gliese 67 38 5.0 1.2 G2 Gliese 668.1 40 6.3 0.4 G9 Gliese 302 41 6.0 0.6 G8 Gliese 309 41 6.4 0.4 K0 Kappa Fornacis 42 5.2 1.3 G1
Gliese 364 45 4.9 1.8 G0 Gliese 599A 45 6.0 0.6 G6 Nu Phoenicis 45 5.0 1.8 F8 Gliese 95 45 6.3 0.5 G5 Gliese 796 47 5.6 0.5 G8 20 Leo Minoris 47 5.4 1.2 G4
www.thelosthaven.co.uk /ZetaIncident.htm   (9627 words)

  
 a fulmination of thought: September 2004   (Site not responding. Last check: 2007-10-08)
Two new "extrasolar" planets (that is, planets outside our Solar System) have been discovered by astronomers, one orbiting the star 55 Cancri, the other orbiting Gliese 436.
Up until now, all of these discoveries of other planets outside our solar system have been of gas giants, like Jupiter, which have little or no chance of evolving and sustaining life as we know it.
- Friedrich Wilhelm Nietzsche (1844-1900) - Die Fröhliche Wissenschaft, Bk III
www.fulmination.com /archive/2004_09_01_archive.html   (1599 words)

  
 [No title]   (Site not responding. Last check: 2007-10-08)
Even if known, it is not immediately evident if companions are physically connected ore only optical.
To cope with this problem Wilhelm Gliese "forgot" the IDS designations.
But, of course, there remain still problem cases where missing information prevent a final decision.
ad.usno.navy.mil /wds/wmc/groupb.txt   (6175 words)

Try your search on: Qwika (all wikis)

Factbites
  About us   |   Why use us?   |   Reviews   |   Press   |   Contact us  
Copyright © 2005-2007 www.factbites.com Usage implies agreement with terms.