NGC 3603 is one of the most massive and densest star clusters within the Milky Way, and can be seen within the constellation of Carina. Around 17 light-years in length, and 20000 light-years away from earth, the cluster can be seen using 7x50 binoculars under good conditions. Its strong ultraviolet radiation and stellar winds have cleared away most of the massive clouds of gas and plasma surrounding it, giving the earth a clear view. The images used to create this picture were taken with the Stocker AstroScience Center 0.61-meter telescope at FIU by Dr. James Webb, and color combined by Bobby Martinez.

Messier 101 is a spiral galaxy more commonly known as the Pinwheel Galaxy and can be seen within the Ursa Major constellation, otherwise known as the Big Dipper constellation. It was discovered by Pierre Mechain on March 27, 1781 and was then verified by Charles Messier as one of his final entries to his Messier Catalogue. As a spiral galaxy it is slightly unusual in the sense that it is viewed face-on from earth. The Pinwheel Galaxy is roughly 170,000 light years in diameter, which is comparable to the diameter of the Milky Way, and is 27 million light years away from earth. It can be observed using only a 3 inch telescope, and on dark moonless nights it can even be spotted with binoculars.

This image is the result of four separate images taken with different wave-lengths filters by the Stocker AstroScience ACE 24” telescope and then reduced and color combined by Bobby Martinez using MIRA Pro.

Messier 64, or commonly known as the Black Eye Galaxy or the Evil Eye Galaxy, is a spiral galaxy that can be located within the Coma Berenices constellation. The “Black Eye” in its name refers to the dark band of dust that obscured the galaxy’s bright central region. In fact the galaxy is actually composed of two counter-rotating disks, the inner disk containing most of the stars and dust, and the outer disk consisting largely of gas. At a distance over 17 million light years from earth the galaxy spans over 70,000 light years. Although catalogued by Charles Messier in 1780, its first known discovery is by Edward Pigott in 1779. The galaxy is easily observed and can be seen with the usage of small telescopes. This image is the result of four separate images taken with different wave-lengths filters by the Stocker AstroScience ACE 24” telescope and then reduced and color combined by Bobby Martinez using MIRA Pro.

VdB 126: The Whispering Lantern of Vulpecula

In the soft darkness of Vulpecula, where star-winds drift like ancient hymns, VdB 126 glows as a delicate reflection nebula — a floating lantern of cosmic dust scattering the blue light of a hidden star. Roughly 1,200 light-years from Earth, this cloud of interstellar grains becomes a quiet teacher of astrophysics, showing how dust not only obscures starlight but also paints it into ethereal color.

This image is the patient sum of 33 frames, each held open for 900 seconds, gathered beneath the night’s long breath. Calibrated with darks, flats, and bias frames, stacked through DeepSkyStacker, and later sculpted in PixInsight and Photoshop, the final portrait reveals both the poetry and the physics of creation.

A reminder that the universe is gentle, luminous, and waiting — if we only dare to look long enough.

What may seem to be a large star in the center this image is actually the Spirograph Nebula (IC 418), shown again blown up in the upper left. It is a planetary nebula that can be seen within the Lepus constellation. At approximately 2000 light-years away and spanning .3 light-years in diameter, the Spirograph Nebula is just too faint to be seen with binoculars. The exact origins and specifics of the nebula are still currently uncertain. The blown up image to the upper left was taken with the Hubble Space Telescope, as the Astroscience Center’s telescope is not powerful enough to take such a close picture. The unusual patterns give the nebula its name, as they resemble patterns drawn using a Spirograph. The individual images was taken by Dr. James Webb at the AstroScience Center on the 16th of January and combined by Bobby Martinez.

Messier 56, a globular cluster within the Lyra constellation, was first discovered by Charles Messier on January 19, 1779. Messier identified his fifty sixth catalogued astronomical object as a “nebula without stars.” Unbeknownst to him it was a 13.7 billion-year-old Class X globular cluster of 80,000 stars. The classification X describes the concentration of stars, with X, or ten, denoting a cluster with a generally loose concentration. The cluster is approximately 32,900 light years away, with a diameter of 84 light years, and is moving towards Earth at 145 kilometers per second. M56 cannot be seen with the unaided eye due to its apparent magnitude of 8.3, but some outer stars can be seen with telescopes with aperture 250mm or larger. It is most discernable in the northern hemisphere from June to August. This image is the final result of four images, with red, green, blue, and luminance filters exposed for 20 seconds. They were taken by Dr. Webb on August 7th, 2015, with FIU’s Stocker AstroScience Center telescope, and were color combined by Gabriel Salazar.

The famous nebula revisited from previous images taken at the Stocker AstroScience Center in Miami Florida on 12/10/2014. The images are 8 second exposures through Johnson R,V and I filters and color combined in Mira to get a psuedo-color image. Although we lack the resolution, even on the best nights, of the Hubble Space telescope, we can still pick up the nebulosity around the central star. This object is a planetary nebula located in the constellation Lepus and is the result of a red giant star which exploded a few million years ago. It is over 3600 light years from Earth and appears to us as a faint nebula only a few arc minutes across in the optical. The famous Space telescope images revealed not only the intricate patterns of nebulosity from which it gained its name "Spirograph Nebula", but also the expansion speed of the gases. The central star was probably very similar to our Sun. These images were taken, re-reduced and color combined by Dr. Webb.

M27, also called the Dumbbell Nebula, is a planetary nebula in the constellation Vulpecula. Charles Messier was the first to discover the object back in 1764. M27 is 1.36 thousand light years away from Earth. The object’s magnitude is around 7.5, making this nebula visible with a low powered telescope during any clear autumn night. In the center of the nebula is a white dwarf star, which is the producer of the gas cloud that surrounds it. The individual images were each exposed for 30 seconds in the R, G, B, and L filters through the FIU AstroScience Center’s 24-inch telescope by physics major Daniel Puentes. The images were then reduced and color-combined by Gabriel Salazar and Daniel Puentes.

Messier 29, discovered in 1764 by Charles Messier, who catalogued over 100 star clusters, nebulae, and galaxies, is an open star cluster in the Cygnus constellation. With an apparent magnitude of 7.1, the cluster can be seen with binoculars or a low-power telescope. It is considered to be relatively young, at 10 million years old. Located 4,000 light years away, M29 contains eight extremely noticeable stars, five of which are classified as B0. This means that, placed in the location of our Sun, any of those five stars would be 160,000 times brighter! This image is the final result of four images, with red, green, and blue filters exposed for 30 seconds, and a luminance filter exposed for 5 seconds. They were taken by Dr. Webb on August 7th, 2015, with FIU’s very own telescope atop the Stocker AstroScience Center, and were color combined by Gabriel Salazar.

Messier 100, which sadly lacks more creative nickname, is a spiral galaxy that can be located within the Coma Berenices constellation. It is approximately 107,000 light years in diameter and is 55 million light years from earth. Messier 100 is also classified as a starburst galaxy, which are galaxies with exceptionally high rate of star formations, with the majority of its star formation concentrated in its bright center. Once again this galaxy is named after Charles Messier for his observation of it in 1781 despite its first known observation being earlier, by Pierre Mechain a month prior.

This image is the result of four separate images taken with different wave-lengths filters by the Stocker AstroScience ACE 24” telescope and then reduced and color combined by Bobby Martinez using MIRA Pro.

Messier 71 is a globular cluster within the constellation Sagitta, which is Latin for “arrow.” It was first discovered by Philippe Loys de Cheseaux in 1746 and was added to the Messier catalogue in 1780. It lies approximately 12,000 light years away and has a diameter of 27 light years. M71 has always been a mystery to astronomers, who have been unable to reach a consensus on the classification of the cluster. It has difficulty fitting into either globular clusters or open clusters, as it is too large, dense, and old (at 9-10 billion years) for open clusters, yet too small, loose, and young for globular clusters. Finally, in the 1970s, during a study of the stars within the cluster, the discovery of the horizontal branch pattern, characteristic of globular clusters, settled the matter. This image is the result of four images, in red, blue, green, and luminance filters, all exposed for thirty seconds. They were taken by physics major Daniel Puentes using the telescope atop FIU’s Stocker AstroScience Center, and were color combined by Gabriel Salazar.

The previously featured Messier 30, a globular cluster within the Capricornus constellation, is the thirtieth object in Charles Messier’s famous catalogue. Discovered in 1764 by Messier himself, the cluster is approximately 12.93 billion years old, 27,000 light years away, and has a diameter of 90 light years. Within this Class V cluster (a moderate concentration towards the center) lies about 150,000 stars! Indeed, a core collapse within M30 has caused the center to become highly dense. Fun fact: Astronomers from the Harvard-Smithsonian Center for Astrophysics have discovered a binary star system about less than one half of a light year from the center. This system includes an extremely dense and small star known as a neutron star, which is the leftover material from a supernova that resulted from the collapse of a massive star. This is the result of four images from red, blue, green, and luminance filters, each exposed for 30 seconds. They were taken by physics major Daniel Puentes with the Stocker AstroScience Center’s telescope and were reduced and color combined by Gabriel Salazar.

Messier 78 is a reflection Nebula that can be located within the Orion constellation. A reflection nebula is one in which clouds of interstellar dust are illuminated by the light of nearby stars, much like fog around a street lamp. It was discovered in 1780 by Pierre Mechain and then documented by Charles Messier. Located over 1600 light years from earth the nebula is roughly 4 light years across. Messier can be spotted even with small telescope or binoculars as a hazy patch near the “belt” of the Orion constellation.

This image is the result of four separate images taken with different wave-lengths filters by the Stocker AstroScience ACE 24” telescope and then reduced and color combined by Bobby Martinez using MIRA Pro.

Physics major Daniel Puentes has started a project of observing the Messier list of objects from the FIU Stocker AstroScience center. To initiate this project, Daniel made images of the globular cluster M107 on July 10, 2015 at the Stocker AstroScience center with the Stocker 24" main telescope. He used RGBL filters and sixty second exposure times to capture the globular cluster located about thirty kilo-light years away from Earth. The images were reduced in MIRA and color combined. This globular cluster is thought to contain about two-hundred-thousand Solar masses of stars within about forty light years.

The initial reductions were done by Daniel Puentes and the final color combination by Dr. Webb.

Messier 76 (M76), also known as the Little Dumbbell Nebula, is a planetary nebula located around 2,500 light years away from Earth. M76 is located in the Perseus nebula with a radius of around 0.617 light years. The name for this particular nebula takes its influence from another planetary nebula (which was a previous astronomy picture of the week!) called the Dumbbell Nebula (M27) due to the shape of the gaseous cloud. The image was taken from the Stocker AstroScience Center at FIU using 60-second exposures in the R, B, G, and L filters by Physics Majors Daniel Puentes and Stephen Revesz. The images were then reduced in MIRA by Daniel Puentes and Stephen Revesz.

Messier 72 is a globular cluster that can be located within the Aquarius constellation. It was first discovered by Pierre Mechain on August of 1780 and was later catalogued by Charles Messier. This star cluster has a diameter of over 100 light years and it is over 55,000 light years away from earth. Due to its distance from earth it is one of the faintest of Messier’s globular clusters, and can barely be seen with smaller telescopes. In fact, when it was first discovered neither Mechain nor Messier could tell what exactly Messier 72 was, thinking it to be a faint nebula.

This image is the result of four separate images taken with different wave-lengths filters by the Stocker AstroScience ACE 24” telescope and then reduced and color combined by Bobby Martinez using MIRA Pro.

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शनि दोष निवारण मंत्र

ऊँ त्रयम्बकं यजामहे सुगंधिम पुष्टिवर्धनम।

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ॐ शन्नोदेवीरभिष्टय आपो भवन्तु पीतये।शंयोरभिश्रवन्तु नः।

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