Weird Science

M45 - The Pleiades, or Seven Sisters

Polish ver­sion is here

The Ple­ia­des, occu­py­ing posi­tion 45 in the Mes­sier cata­log (M45), is argu­a­bly the most well-known open star clu­ster in the night sky. It is loca­ted in the con­stel­la­tion Tau­rus, appro­xi­ma­tely 444 light-years from Earth.

Seve­ral stars within the clu­ster have indi­vi­dual names lin­ked to the Greek myth of the Ple­ia­des. Accor­ding to mytho­logy, they were the seven dau­gh­ters of the Titan Atlas and the Oce­a­nid Ple­ione, and the sisters of the Hya­des (which were also pla­ced in the sky as a sepa­rate open clu­ster). Among the Ple­ia­des, we find Tay­geta, Maia, Aste­rope, Ste­rope II, Merope, Alcy­one, Cela­eno, and Elec­tra, as well as their reve­red parents. The fact that eight Ple­ia­des are listed today instead of seven is due to the histo­ri­cal gro­u­ping of Aste­rope and Ste­rope II under a sin­gle name.

The clu­ster was also reco­gni­zed in various cul­tu­res and often held signi­fi­cant roles in local beliefs. For this rea­son, these stars are known by nume­rous other names, inc­lu­ding the Chicks, the Seven Sisters, and even the Maso­nic Church. In some Eastern Sla­vic lan­gu­a­ges, such as Ukra­i­nian (Стожари) and Rus­sian (Стажары), as well as in older Polish lite­ra­ture, they are some­ti­mes refer­red to as Sto­zhary (pol. Sto­żary).

The theme of the Ple­ia­des has also been explo­red in lite­ra­ture. Along­side other stel­lar gro­u­ping­s—the Hya­des and the Dou­ble Clu­ster in Per­seu­s—they play an impor­tant role in Ser­gey Sne­gov’s sci-fi cycle Peo­ple as Gods (Rus­sian: Люди как боги). Addi­tio­nally, in the works of H.P. Love­craft and the Cthulhu Mythos, the Ple­ia­des are men­tio­ned in refe­rence to the Great Library, an ancient repo­si­tory of know­ledge said to be loca­ted on Cela­eno or a pla­net orbi­ting it.

Obse­rva­tions

Janu­ary 12, 2020 – Jaworzno (Poland), gar­den
urban con­di­tions, high level of light pol­lu­tion

The Ple­ia­des can be easily loca­ted in the night sky by exten­ding the line con­nec­ting Bel­la­trix (Gamma Orio­nis, γ Ori) and Alde­ba­ran (Alpha Tauri, α Tau) bey­ond Alde­ba­ran toward the nor­th­west. The best con­di­tions for obse­rving this clu­ster in Poland occur from Octo­ber to March, making the begin­ning of the yea­r—such as in this case­—an excel­lent time.

The shape for­med by the bri­gh­test stars visi­ble to the naked eye in the clu­ster may resem­ble a minia­ture ver­sion of the Big Dip­per aste­rism.

The clu­ster con­ta­ins seve­ral hun­dred stars. Most of them are blue giants of spec­tral type B. Their appa­rent magni­tu­des range from 3.0m to 5.9m, and they are rela­ti­vely young stars, with an esti­ma­ted age of appro­xi­ma­tely 100 mil­lion years.




Sep­tem­ber 19, 2020 – Jaworzno (Poland), gar­den
urban con­di­tions, high level of light pol­lu­tion

Here they are! The Ple­ia­des have retur­ned to the night sky! The beau­ti­ful sisters, along with their parent­s—the Tita­ness Ple­ione and the Titan Atlas, who, as we know from Greek mytho­logy, was tasked with car­ry­ing the cele­stial sphere on his sho­ul­ders.

After seve­ral mon­ths of absen­ce­—ro­u­ghly since late Mar­ch—the Ple­ia­des are once again visi­ble for incre­a­sin­gly long periods at night, allo­wing obse­rvers to admire this magni­fi­cent open clu­ster without the need for a tele­scope or any opti­cal aids.

While the Ple­ia­des can easily be seen with the naked eye under dark skies, bino­cu­lars pro­vide a signi­fi­can­tly enhan­ced vie­wing expe­rience. Howe­ver, much more intri­cate deta­ils become visi­ble only in long-expo­sure pho­to­gra­phs. The pre­sen­ted image was taken rather spon­ta­ne­o­u­sly from an area with high levels of light pol­lu­tion, without a tele­scope, near the time of the full Moon and in its rela­ti­vely close pro­xi­mity.

It was a ple­a­sant sur­prise to see that even in such a sub­op­ti­mal pho­to­graph, taken under dif­fi­cult con­di­tions, the deli­cate outline of the beau­ti­ful blue nebula enve­lo­ping the stars in this clu­ster could still be discer­ned.




Decem­ber 6, 2021 – Jaworzno (Poland), gar­den
urban con­di­tions, high level of light pol­lu­tion

This time, the obse­rving con­di­tions were ide­a­l—the night was moon­less, quite cold, and the sky rema­i­ned clear long eno­ugh to col­lect suf­fi­cient data.

Thanks to bet­ter con­di­tions and a lon­ger expo­sure time than in Photo 2, we can now more cle­arly see the stun­ning set of reflec­tion nebu­lae illu­mi­na­ted by the blue glow of young, hot stars. Nota­ble among them is the Merope Nebula (NGC 1435, also known as Tem­pel’s Nebula) and the nebula sur­ro­un­ding Maia (NGC 1432). These beau­ti­ful clo­uds of gas and dust may be rem­nants of the mole­cu­lar cloud from which the clu­ster's stars for­med, altho­ugh other ori­gins are also pos­si­ble. The stri­king blu­ish hue of these nebu­lae results from the pre­sence of fine car­bo­na­ce­ous dust scat­te­red thro­u­ghout this region of space.




Photo 1 Para­me­ters:

  • Total expo­sure time: 10 seconds (sin­gle shot)
  • Canon EOS 60D
  • ISO: 1500
  • Lens: zoom type (used at fmax = 250mm)
  • 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.

Photo 2 Para­me­ters:

  • Total expo­sure time: 15 minu­tes (stack of 15 RAW fra­mes at 60s each, using an appro­priate num­ber of dark, bias, and flat fra­mes)
  • Canon EOS 60D
  • ISO: 500
  • Lens: zoom type (used at fmax = 250mm)
  • 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.

Photo 3 Para­me­ters:

  • Total expo­sure time: 28 minu­tes (stack of 14 RAW fra­mes at 120s each, using an appro­priate num­ber of dark, bias, and flat fra­mes)
  • Canon EOS 60D
  • ISO: 1500
  • Lens: zoom type (used at fmax = 250mm)
  • 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.

Marek Ples

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