Weird Science

M31 (M32, M101) – the Andromeda Galaxy and its satellite galaxies

Polish ver­sion is here

The Andro­meda Galaxy (M31 in the Mes­sier cata­log) is loca­ted in the con­stel­la­tion Andro­meda, named after the mytho­lo­gi­cal prin­cess, the dau­gh­ter of King Cepheus of Ethio­pia. Its distance from Earth is appro­xi­ma­tely 2.52 mil­lion light-years.

It is the lar­gest and bri­gh­test exter­nal galaxy visi­ble in the nor­thern sky. Under favo­ra­ble con­di­tion­s—far from the light pol­lu­tion of urban are­a­s—its bri­gh­test cen­tral regions can often be seen with the naked eye as a small, sli­gh­tly fuzzy star or a faint patch of light. Howe­ver, to fully appre­ciate its beauty, appro­priate opti­cal equ­ip­ment is requ­i­red.

The Andro­meda Galaxy is clas­si­fied as an Sb galaxy in Hub­ble’s clas­si­fi­ca­tion or SA(s)b in the revi­sed sys­tem, mea­ning it is a spi­ral galaxy without a cen­tral bar, fea­tu­ring a medium-sized core and well-deve­lo­ped spi­ral arms. Howe­ver, scien­ti­fic reports from 2006 sug­gest that M31 may have a small bar, which would clas­sify it as SAB(s)b. Addi­tio­nally, Andro­meda is cate­go­ri­zed as a Low-Ioni­za­tion Nuc­lear Emis­sion-line Region (LINER), pla­cing it in the most com­mon group of gala­xies with active nuc­lei.

The Andro­meda Galaxy has a dense dou­ble core con­ta­i­ning at least one black hole, at least two spi­ral arms accom­pa­nied by a ring of cosmic dust (which may ori­gi­nate from the smal­ler galaxy M32), and more than 450 glo­bu­lar clu­ster­s—some of which are among the den­sest known.

Inte­re­stin­gly, 14 dwarf satel­lite gala­xies have been iden­ti­fied orbi­ting Andro­meda, the most well-known being M32 and M110.

Obse­rva­tions

August 17, 2018 – Jaworzno (Poland), gar­den
urban con­di­tions, high level of light pol­lu­tion

The peak period for obse­rving mete­ors from the Per­seid meteor sho­wer is slowly coming to an end, but that doesn’t mean the night sky above our heads has become any less inte­re­sting. On the con­trary, late sum­mer and early autumn pro­vide excel­lent oppor­tu­ni­ties to obse­rve many fasci­na­ting deep-sky objects. One of them is the Andro­meda Galaxy.

The pho­to­gra­phs belo­w—both the ori­gi­nal and its anno­ta­ted ver­sio­n—were taken without the use of a tele­scope. I used an older Canon EOS 300D DSLR with a 250mm tele­photo lens. The final image is a stack of 10 expo­su­res, each with a 120-second expo­sure time, resul­ting in a total expo­sure of appro­xi­ma­tely 20 minu­tes (of course, for stac­king pur­po­ses, the requ­i­red num­ber of dark and flat fra­mes was also cap­tu­red). This was my first pho­to­graph of this object, and unfor­tu­na­tely, it is some­what blurry due to an acci­den­tal mis­fo­cus while adju­sting the camera. None­the­less, I have great sen­ti­men­tal value atta­ched to this photo.

The pho­to­graph shows the Andro­meda Galaxy, a beau­ti­ful exam­ple of a spi­ral galaxy. Its struc­tu­ral ele­ments are cle­arly visi­ble, such as the bri­ght cen­tral bulge and the galac­tic disk. Dark bands within the disk (mar­ked with arrows) are also noti­ce­a­ble. Addi­tio­nally, two other extra­ga­lac­tic star sys­tem­s—na­mely the dwarf gala­xies M32 and M110—are distinc­tly visi­ble. Both are satel­li­tes of the Andro­meda Galaxy, orbi­ting aro­und it. Sli­gh­tly below is the star ν Andro­me­dae (Nu Andro­me­dae), a spec­tro­sco­pic binary star whose com­po­nents orbit their com­mon cen­ter of mass with a period of just over four Earth days.




Sep­tem­ber 5, 2019 – Jaworzno (Poland), gar­den
urban con­di­tions, high level of light pol­lu­tion

Just over a year after my pre­vious attempt at pho­to­gra­phing M31, and having upgra­ded to a newer camera (Canon EOS 60D), I plan­ned ano­ther ses­sion.

As seen, the image sharp­ness is signi­fi­can­tly bet­ter, reve­a­ling more deta­ils of the galaxy’s struc­ture and the dark lanes within its spi­ral arms. The lon­ger expo­sure time hel­ped high­li­ght a gre­a­ter num­ber of deta­ils. The above pho­to­graph is crop­ped; the ori­gi­nal image is pre­sen­ted below:

The view of this distant stel­lar sys­tem, suspen­ded in an incom­pre­hen­si­bly vast cosmic void, never fails to make me pon­der the myste­ries of the uni­verse.

Photo 1 Para­me­ters:

  • Total expo­sure time: 20 minu­tes (stack of 10 RAW fra­mes at 120s each, using an appro­priate num­ber of dark, bias, and flat fra­mes)
  • Canon EOS 60D
  • ISO: 2500
  • Fake colors
  • Lens: zoom type (used at fmax = 250mm)
  • Aper­ture: f/4 (the smal­lest pos­si­ble for the lens used)
  • Mount: equ­a­to­rial mount with trac­king, ali­gned using the drift method and con­trol­led by a custom-built sys­tem

Pho­tos 2 and 3 Para­me­ters:

  • Total expo­sure time: 36 minu­tes (stack of 36 RAW fra­mes at 60s each, using an appro­priate num­ber of dark, bias, and flat fra­mes)
  • Canon EOS 60D
  • ISO: 800
  • Lens: zoom type (used at fmax = 250mm)
  • Aper­ture: f/4 (the smal­lest pos­si­ble for the lens used)
  • Mount: equ­a­to­rial mount with trac­king, ali­gned using the drift method and con­trol­led by a custom-built sys­tem

Marek Ples

Aa