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The Bubble Nebula NGC 7635 Sharpless 162 Binder

$23.10

per binder

Qty:
1
15% Off with code ZAZZLESAVING
  • Background
    Background
  • Front/Inside
    Front / Inside
  • Front
    Front
  • Back
    Back
  • Spine
    Spine
  • Front/Spine
    Front / Spine
  • Back/Spine
    Back / Spine
The Bubble Nebula NGC 7635 Sharpless 162 Binder
Designed for youby wallarts
Avery Signature 1" Binder
Size
Select an option:
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Avery Signature 1" Binder
 
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Avery Signature 1.5" Binder
 
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Avery Signature 2" Binder
+ $2.25
About This Product
  • Sold by
Size: Avery Signature 1" Binder

You’ve spent time crafting interesting reports, so why not create an eye-catching Avery custom binder to match? Showcase your business with custom client binders, proposals and reports, or design unique wedding albums, recipe books and photo albums.

  • Dimensions: 10"l x 11.75"w; Spine: 1.4"
  • Full bleed photo-quality printing
  • Designed for letter (8.5" x 11") sized paper
  • Fits 275 pages with 1 Touch™ EZD™ Rings
  • Binder inserts not included
  • Made in U.S.A.
  • Designer Tip: To ensure the highest quality print, please note that this product’s customizable design area measures 10.55" x 11.6". For best results please add 1/4" bleed.
This product is recommended for ages 6+
Ring Type: One Touch EZD™ Ring
1" Capacity: 275 pages
1.5" Capacity: 400 pages
2" Capacity: 540 pages
Locking rings open with ease and keep pages secure.
About This Design
available on 48 products
The Bubble Nebula NGC 7635 Sharpless 162 Binder
NGC 7635, also called the Bubble Nebula, Sharpless 162, or Caldwell 11, is a H II region emission nebula in the constellation Cassiopeia. It lies close to the direction of the open cluster Messier 52. The "bubble" is created by the stellar wind from a massive hot, 8.7 magnitude young central star, the 15 ± 5 M☉ SAO 20575 (BD+60 2522). The nebula is near a giant molecular cloud which contains the expansion of the bubble nebula while itself being excited by the hot central star, causing it to glow. It was discovered in 1787 by Friedrich Wilhelm Herschel. The star SAO 20575 or BD+602522 is thought to have a mass of 10-40 Solar masses. All Rights Reserved; without: prejudice, recourse or notice (U.C.C. 1-308)
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