NGC 4214 is a dwarf barred irregular galaxy located about 10 million light years away in the constellation Canes Venatici. It is famed for its intense star formation activity, with vibrant blue star clusters and pink nebulae, similar to the Orion Nebula in our Milky Way. Captured by Ron Brecher (@astrodoc.ca) with his Celestron EdgeHD 1400 telescope for a total of 8hr 45m. 15 x 5m Red = 1hr 15m 12 x 5m Green = 1hr 00m 16 x 5m Blue = 1hr20m 44 x 5m Lum = 3hr40m 18 x 5m Ha = 1hr 30m
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Possible TLP seen by TGE Elger with a Cooke telescope in 1867 https://lnkd.in/erzWesiX
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Gamma Argus (Vela) observed with a Cooke telescope https://lnkd.in/e5yiKUS3
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The C/2023 A3 Tsuchinshan-Atlas comet, as seen from Barcelona through a 4 cm telescope in a 5-minute exposure. Field of view is 11°x7°, meaning, the tail is huge! This is one of the very few comets that has developed an anti-tail, made of the heavier dust particles that are immune to the solar-wind push (https://lnkd.in/diFGXb7C). In the photo, you can see the anti-tail as a spike in front of the comet's coma.
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This Hubble Telescope image showcases the visually striking nebula RCW 7, located over 5,300 light-years away in the constellation Puppis.Nebulae are areas rich in the raw material needed to form new stars. Under the influence of gravity, parts of these molecular clouds collapse until they coalesce into very young, developing stars, called protostars, continue... https://lnkd.in/guSErNtH
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5 amazing things discovered by the eROSITA X-ray telescope https://lnkd.in/gv2CawvK #amazing #discovered #erosita #telescope #xray
5 amazing things discovered by the eROSITA X-ray telescope
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Messier 13 (M13 or NGC 6205) is also referred to as the Great Globular Cluster in Hercules, is one of the brightest and best known globular clusters in the northern skies. It shines at a magnitude of 5.8, is about 22,200 light years away and contains an estimated 300,000 stars. Observation data (J2000 epoch) Class: V Constellation: Hercules Right ascension: 16h 41m 41.24s Declination: +36° 27′ 35.5″ Distance: 22.2 kly Apparent magnitude (V): 5.8 Apparent dimensions (V): 20 arcminutes Tech Specs: Orion 8” RC Telescope, ZWO ASI2600MC camera running at -10F, 2h30m using 60 second exposures, Celestron CGEM-DX pier mounted, ZWO EAF and ASIAir Plus, processed in PixInsight. Image Date: April 15, 2024. Location: The Dark Side Observatory (W59), Weatherly, PA, USA (Bortle Class 4).
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🔆〰 Light is energy and can take many forms. Colors are merely the way our brain interpret the wavelength of light. However, the human eye can only see one tenth of a billion of the electromagnetic spectrum, which ranges from radio waves to gamma rays. Many insects can see ultraviolets, while some fish, reptiles, and amphibians can see infrared radiation. There's a whole world around us that simply isn't within reach of our eyes, but the same cannot be said of our intellect: just consider the applications of X-rays or UV radiation, for example, or how the James Webb Space Telescope has revolutionized the image we have of the universe by recording it with its Near-Infrared Camera (NIRCam) 🔭🪐✨ www.arquiled.com #Arquiled #constructelvisabeira
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5 amazing things discovered by the eROSITA X-ray telescope https://lnkd.in/gv2CawvK #amazing #discovered #erosita #telescope #xray
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With revised technique and calculations, I found that the faintest star visible in this frame is of magnitude 13.8 (see comment below). So I reasonably estimated the debris streak at 1 magnitude fainter. Had the telescope been tracking the debris, it would have stayed on one (binned) pixel in the 200ms exposure, appearing as an object of magnitude 9 (calculated separately/updated), giving it a size of approximately 10-11cm at its calculated altitude of 445km (calculated from the length of the streak against the FOV and exposure). This is fairly close to our target of achieving detection of 10cm or smaller LEO objects.
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The Moon was low in the south west. it was too low for my telescope, so I used my DSLR at 300mm focal length, ISO 100 and 1/500 second exposure. https://lnkd.in/eT-remav
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