M101

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M101

🎯 Target: M101

📅 Date: 17 Giugno 2026

🏷️ Category: Galaxies

📍 Location: Milano

⚙️ Acquisition Setup

  • 🔭 Optics: William Optics RedCat 61
  • 📸 Sensor: ASI 585MC AIR
  • ⏱️ Exposure: 60,0 min
  • Gain: 150

Processing Notes

**Object:** Messier 101 (M101) / NGC 5457
**Common Name:** The Pinwheel Galaxy
**Type:** Grand Design Spiral Galaxy
**Constellation:** Ursa Major

Messier 101 is one of the most striking examples of a "grand design" spiral galaxy in the night sky. Viewed nearly precisely face-on from Earth, it reveals a dazzling, intricate structure of tightly wound spiral arms, glowing nebulae, and vast star-forming regions. Because of its large size and low surface brightness, it can be a delightful challenge for visual observers but rewards astrophotographers with incredible detail.

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### **Key Data**

* **Distance:** Approximately 21 million light-years
* **Visual Magnitude:** 7.8
* **Apparent Size:** 28.8 x 26.9 arcminutes
* **Actual Diameter:** Around 170,000 light-years (nearly twice the size of our Milky Way)

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### **Fast Facts & Curiosities**

* **A Massive Giant:** M101 is enormous. It is estimated to contain at least one trillion stars, vastly outnumbering the population of the Milky Way.
* **Asymmetrical Beauty:** The galaxy's spiral arms are noticeably asymmetrical. This warping is caused by intense gravitational tidal forces from recent cosmic encounters with its smaller companion galaxies (NGC 5474, NGC 5477, and others).
* **Supernova Hotspot:** In recent decades, M101 has hosted several high-profile supernovae. The most recent notable event was SN 2023ixf, a Type II supernova discovered in May 2023, which became bright enough to be easily captured by amateur equipment.
* **H II Hyper-regions:** The spiral arms are packed with giant H II regions (areas of ionized hydrogen gas). In fact, M101 contains some of the largest star-forming regions known, so prominent that several of them have their own independent NGC designations (like NGC 5461 and NGC 5462).

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### **Observing Tips**

While its integrated magnitude is 7.8, M101 spreads that light over an area nearly the size of the full Moon. Under dark skies, binoculars or a small telescope will reveal its bright core as a hazy patch. To resolve the magnificent spiral arms or spot the massive H II knots within them, a larger aperture or long-exposure astrophotography is required.