NGC4689 - HST - Potw2007a
However, seen almost face on, NGC 4689 appears less like a majestic spiral and more like a smudged fingerprint on the sky. No matter how good the image quality, there is little contrast between the spiralling arms of stars, gas, and dust, and the less dense areas in between. This is because NGC 4689 is something known as an “anaemic galaxy”, a galaxy that contains only quite small quantities of the raw materials needed to produce stars. This means that star formation is quelled in NGC 4689, and the pinwheeling, bustling arms are less bright than those belonging to other Hubble muses.
Despite this subtlety when compared to its brash, spotlight-stealing relatives, NGC 4689 retains an otherworldly charm, its delicately glowing material standing out subtly from the surrounding darkness of space.Relevante Bilder
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NGC 4689NGC 4689 ist eine Spiralgalaxie mit aktivem Galaxienkern vom Hubble-Typ Sbc im Sternbild Coma Berenices am Nordsternhimmel. Sie ist schätzungsweise 70 Millionen Lichtjahre von der Milchstraße entfernt und hat einen Durchmesser von etwa 95.000 Lichtjahren. Unter der Katalognummer VCC 2058 wird sie als Mitglied des Virgo-Galaxienhaufens geführt. .. weiterlesen