Weird Science

M66 - Barred Spiral Galaxy in Leo

Polish ver­sion is here

Mes­sier 66 (M66), also cata­lo­ged as NGC 3627 or Arp 16, is one of seve­ral spi­ral gala­xies that grace the spring skies in the con­stel­la­tion Leo. Loca­ted about 36 mil­lion light-years (≈11 Mpc) from Earth, it was disco­ve­red on March 1, 1780, by Char­les Mes­sier.

Obse­rva­tions

April 26, 2025, aro­und 2:00 AM – Jaworzno, Poland
Con­di­tions: high light pol­lu­tion

The night was clear, altho­ugh the sky appe­a­red sli­gh­tly hazy. Toward the end of the ses­sion a few iso­la­ted clo­uds dri­fted thro­ugh, but they did not hin­der the obse­rva­tions.

M66 is part of the famous Leo Tri­plet (Arp 317) — a tight group of three gra­vi­ta­tio­nally inte­rac­ting gala­xies that also inc­lu­des M65 and NGC 3628 (Photo 1).

Span­ning nearly 96,000 light-years across, M66 exhi­bits well-defi­ned spi­ral arms rich in inter­stel­lar dust. Along those arms lie nume­rous bri­ght clu­sters of young stars, proof that vigo­rous star for­ma­tion is still under way. The arms, howe­ver, are noti­ce­a­bly asym­me­tric: one side of the disk appe­ars more stret­ched and distor­ted, hin­ting at past or ongo­ing gra­vi­ta­tio­nal enco­un­ters with nei­gh­bo­ring gala­xies.

Seve­ral super­no­vae have been recor­ded in M66. SN 1973R and SN 1989B were clas­sic stel­lar explo­sions, whe­reas SN 1997bs tur­ned out to be a likely impo­stor — a stel­lar out­burst that ini­tially appe­ars to be a super­nova but does not destroy its pro­ge­ni­tor star. The most recent event, SN 2009hd, again con­fir­med that M66 still har­bors young, mas­sive stars desti­ned for spec­ta­cu­lar endings.

Photo 1 Para­me­ters:

  • Total expo­sure time: 90 minu­tes (stack of 90 RAW fra­mes at 60s each, using an appro­priate num­ber of dark, bias, and flat fra­mes)
  • ISO: 1600
  • Mak­su­tov-Cas­se­grain tele­scope (100/1400), prime focus expo­sure
  • A fil­ter was used to reduce the effects of arti­fi­cial light pol­lu­tion and atmo­sphe­ric glow
  • Mount: equ­a­to­rial mount with trac­king, ali­gned using the drift method and con­trol­led by a custom-built sys­tem.

Fur­ther rea­dings:

Marek Ples

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