It has an apparent diameter of 20 arcseconds, with small scopes revealing a star-like object at low magnification. Upping the power won’t show detail, but should reveal the elliptical shape of this planetary. To help you find the objects on our tour, download our PDF chart of deep-sky objects around Orion’s Head. The Flame Nebula needs dark skies and low magnification to see well. Use a 6-inch reflector, making sure you keep nearby Alnitak out of the field of view to improve contrast, and you should be able to see its mottled fan shape.
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This has a similar size to our previous target, but is slightly brighter with a listed integrated magnitude of +8.5. This little planetary nebula can be found just southeast of mag. In a 6-inch Dobsonian it is small and round, appearing a pale greenish-blue.
Rigel (Beta Orionis)
This is an image of Orion in the night sky, with lines showing where south, east and west are in relation to it. Dive into the world of stargazing with our comprehensive guide to the constellations! 🌠 Find out everything you need to know about star patterns you see in the night sky. The constellation Orion is prominently visible in the evening sky from November to early May, with its peak observation period occurring between January and April. During these months, Orion rises to its highest point and remains visible throughout the night. Additionally, it can be seen in the morning sky from late July to Orions bet November.
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- Four stars—Rigel, Betelgeuse, Bellatrix, and Saiph—form a large roughly rectangular shape, at the center of which lie the three stars of Orion’s Belt—Alnitak, Alnilam, and Mintaka.
- +6.8 star 52 arcseconds to the north of the primary and a far fainter 14th magnitude star in between.
- It occupies a roughly circular area 6.5˚ across, centred on Meissa and has low surface brightness, with the brightest part west of Meissa.
- Some parts of their surfaces are contracting while others simultaneously expand.
- +5.2 45 Orionis sits north of the Orion Nebula (M42) and the adjacent De Mairan’s Nebula (M43), which itself is above mag.
Alnitak
- The Trapezium cluster (Theta1 Orionis) is an open cluster located in the heart of the Orion Nebula.
- Orion’s Belt is a line of three stars located around the middle of the constellation Orion.
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The count increases to around 20 cluster members through a 300mm telescope. This barred face-on spiral galaxy has a stated magnitude range of mag. See if you can detect it with a 14-inch Newtonian at 200x magnification as a faint roundish smudge of light. One of the easier ones to find is NGC 1924, which lies to the west of M42, shines at mag. +13.3 and may be as far as 100 million lightyears away.
Middle East
It is the faintest star of Orion’s Belt and the only one that is not a supergiant. Both amateur stargazers and skilled astronomers are familiar with Orion’s Belt, which is a prominent star pattern often used for navigating the sky. It consists of three evenly-spaced stars that form a nearly straight line. They were probably all born around the same time and formed from the plasma clouds within the same sky region we now know as Orion’s belt. +4.4 Pi2 (π2) Orionis to home in on this faint galaxy, which rests just 18 arcminutes east of the star and shines at mag.
A line extended from the Belt stars to the southeast leads to Sirius, the brightest star in the sky. Popularly known as the Dog Star, Sirius is the brightest star in the constellation Canis Major and one of the nearest stars to the Sun. The primary component (Delta Ori Aa1) is part of a triple star system that also contains a hot blue B-type main sequence star (Delta Ori Aa2) and a B-type subgiant star (Delta Ori Ab). The closer companion, Delta Orionis Aa2, has a mass of 8.4 solar masses and a radius 6.5 times that of the Sun.
