NGC 6503

Galaxie
NGC 6503
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Aufnahme mithilfe des Hubble-Weltraumteleskops
AladinLite
SternbildDrache
Position
ÄquinoktiumJ2000.0, Epoche: J2000.0
Rektaszension17h 49m 26,432s[1]
Deklination+70° 08′ 39,72″[1]
Erscheinungsbild
Morphologischer TypSA(s)cd / HII / LINER[1]
Helligkeit (visuell)10,2 mag[2]
Helligkeit (B-Band)10,9 mag[2]
Winkel­ausdehnung7,1′ × 2,4′[1]
Positionswinkel123°[2]
Inklination°
Flächen­helligkeit13,2 mag/arcmin²[2]
Physikalische Daten
Zugehörigkeitisoliert
NGC 6503-Gruppe[1]
Rotverschiebung0,000083 ± 0,000003[1]
Radial­geschwin­digkeit(25 ± 1) km/s[1]
Hubbledistanz
H0 = 73 km/(s • Mpc)
(16 ± 3) · 106 Lj
(4,927 ± 0,997) Mpc [1]
Absolute Helligkeitmag
MasseM
Durchmesser35.000 Lj
Metallizität [Fe/H]{{{Metallizität}}}
Geschichte
EntdeckungArthur Auwers
Entdeckungsdatum22. Juli 1854
Katalogbezeichnungen
NGC 6503 • UGC 11012 • PGC 60921 • CGCG 340-019 • MCG +12-17-009 • IRAS 17499+7009 • 2MASX J17492651+7008396 • GC 4351 • 2MASS J17492642+7008395 • KIG 837 • 2MIG 2437

NGC 6503 ist eine aktive Spiralgalaxie mit ausgedehnten Sternentstehungsgebieten (im Foto rot) vom Hubble-Typ Sc im Sternbild Drache am Nordsternhimmel. Sie ist schätzungsweise 16 Millionen Lichtjahre von der Milchstraße entfernt und hat einen Durchmesser von etwa 37.000 Lichtjahren.

Die Galaxie liegt einzeln im Lokalen Void, einer riesigen, leeren Region des Weltraums neben unserer lokalen Gruppe.

Hellblaue Regionen enthalten neu entstehende Sterne. Dunkelbraune Staubstreifen winden sich über die hellen Arme und die Mitte der Galaxie und geben ihr ein fleckiges Aussehen.

Das Objekt wurde am 22. Juli 1854 von dem deutschen Astronomen Arthur Auwers (1838–1915) entdeckt, und zwar noch als Schüler, rund drei Wochen vor seinem 16. Geburtstag.[3]

Literatur

  • König, Michael & Binnewies, Stefan (2019): Bildatlas der Galaxien: Die Astrophysik hinter den Astrofotografien, Stuttgart: Kosmos, S. 100

Einzelnachweise

  1. a b c d e f NASA/IPAC EXTRAGALACTIC DATABASE
  2. a b c d SEDS
  3. Seligman

Auf dieser Seite verwendete Medien

Lonely Galaxy Lost in Space (18059364654).jpg

Most galaxies are clumped together in groups or clusters. A neighboring galaxy is never far away. But this galaxy, known as NGC 6503, has found itself in a lonely position, at the edge of a strangely empty patch of space called the Local Void.

The Local Void is a huge stretch of space that is at least 150 million light-years across. It seems completely empty of stars or galaxies. The galaxy’s odd location on the edge of this never-land led stargazer Stephen James O’Meara to dub it the “Lost-In-Space galaxy” in his 2007 book, Hidden Treasures.

NGC 6503 is 18 million light-years away from us in the northern circumpolar constellation of Draco. NGC 6503 spans some 30,000 light-years, about a third of the size of the Milky Way.

This Hubble Space Telescope image shows NGC 6503 in striking detail and with a rich set of colors. Bright red patches of gas can be seen scattered through its swirling spiral arms, mixed with bright blue regions that contain newly forming stars. Dark brown dust lanes snake across the galaxy’s bright arms and center, giving it a mottled appearance.

The Hubble Advanced Camera for Surveys data for NGC 6503 were taken in April 2003, and the Wide Field Camera 3 data were taken in August 2013.

The Hubble Space Telescope is a project of international cooperation between NASA and the European Space Agency. NASA’s Goddard Space Flight Center in Greenbelt, Maryland, manages the telescope. The Space Telescope Science Institute (STScI) in Baltimore conducts Hubble science operations. STScI is operated for NASA by the Association of Universities for Research in Astronomy, Inc., in Washington, D.C.

Photo Credit: NASA, ESA, D. Calzetti (University of Massachusetts), H. Ford (Johns Hopkins University), and the Hubble Heritage Team

NASA image use policy.

NASA Goddard Space Flight Center enables NASA’s mission through four scientific endeavors: Earth Science, Heliophysics, Solar System Exploration, and Astrophysics. Goddard plays a leading role in NASA’s accomplishments by contributing compelling scientific knowledge to advance the Agency’s mission.

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NGC 6503 HST.jpg
Fresh starbirth infuses the galaxy NGC 6503 with a vital pink glow in this image from the NASA/ESA Hubble Space Telescope. This galaxy, a smaller version of the Milky Way, is perched near a great void in space where few other galaxies reside.

This new image from Hubble’s Advanced Camera for Surveys displays, with particular clarity, the pink-coloured puffs marking where stars have recently formed in NGC 6503's swirling spiral arms. Although structurally similar to the Milky Way, the disc of NGC 6503 spans just 30 000 light-years, or just about a third of the size of the Milky Way, leading astronomers to classify NGC 6503 as a dwarf spiral galaxy.

NGC 6503 lies approximately 17 million light-years away in the constellation of Draco (the Dragon). The German astronomer Arthur Auwers discovered this galaxy in July 1854 in a region of space where few other luminous bodies have been found.

NGC 6503 sits at the edge of a giant, hollowed-out region of space called the Local Void. The Hercules and Coma galaxy clusters, as well as our own Local Group of galaxies, circumscribe this vast, sparsely populated region. Estimates for the void’s diameter vary from 30 million to more than 150 million light-years — so NGC 6503 does not have a lot of galactic company in its immediate vicinity.

The isolation of NGC 6503 inspired the stargazer Stephen James O'Meara to name it the Lost-In-Space Galaxy in his book Hidden Treasures.

This Hubble image was created from exposures taken with the Wide Field Channel of the Advanced Camera for Surveys. The filters were unusual, which explains the peculiar colour balance of this picture. The red colouration derives from a 28-minute exposure through a filter that just allows the emission from hydrogen gas (F658N) to pass and which reveals the glowing clouds of gas associated with star-forming regions. This was combined with a 12-minute exposure through a near-infrared filter (F814W), which was coloured blue for contrast. The field of view is 3.3 by 1.8 arcminutes.