Astrofotografia
View allAll Photos Tagged astrofotografia
Las fronteras son líneas imaginarias.
Frontera entre Cáceres, comarca de Alcántara y Portugal en el puente de Segura.
Border between Spain in Portugal at Segura Bridge, close to Alcántara.
Star Trails over my hometown Valencia de Alcántara, Caceres, Extremadura, Spain.
Estelas de estrellas sobre mi pueblo Valencia de Alcántara, Cáceres, Extremadura, España
CATEGORY: Stacked
SOCIAL IG: @victorlimaphoto
STORY:
Even so being born in the Espírito Santo state/Brazil, I had never photographed the night landscapes of my state.
Yesterday I had the opportunity to visit and photograph the surroundings of Pedra Azul, in the mountain region of Espírito Santo. It was a wonderful experience and the quality of the region's sky for landscape astrophotography can be seen in the image above.
Image maded using the stacking technique for noise reduction. Sky and terrain captured at the same moment.
EXIF:
Canon 6Da | EF 16-35mm f/2.8L II
7x 24mm | 15 sec | f/2.8 | ISO 8000
#victorlimaphoto #astrofotografia #milkyway #vialactea #pedraazul #vitoria #vilavelha #espiritosanto
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Gamma Cygni lies at the center of the Northern Cross
Imaging telescope: Vixen VSD 100 f/3
Imaging camera: 9.2mp Sony SX814
Mount: Software Bisque Paramount MX
Guiding telescope or lens: Vixen VSD 100 f/3
Filters: Chroma SII 3nm, Chroma OIII 3nm, Chroma Ha 3nm
Accessories: Chroma OIII 3nm, Chroma Ha 3 nm
Frames:12x1800"x3
Integration: 18 hours
Entre encinas y megalitos
Dolmen Tapada del Anta, Valencia de Alcántara, Cáceres, Extremadura, España. (Spain)
Fase Cuarto creciente.
La media luna de cera del 8 de noviembre tiene una iluminación del 18%. Este es el porcentaje de la Luna iluminada por el Sol. La iluminación cambia constantemente y puede variar hasta un 10% al día. El 8 de noviembre la Luna tiene 4,14 días. La luna está cerca del sol en el cielo y en su mayor parte oscura, excepto por el borde derecho de la luna, que se vuelve más brillante a medida que los días se acercan a la siguiente fase, que es un primer trimestre con un 50% de iluminación.
Detalles de fase para - 8 de noviembre Fase:
Creciente
iluminación creciente: 18% Edad lunar: 4,14 días
Ángulo lunar: 0,55
Distancia lunar: 364.897,83 km
Ángulo solar: 0,54
Distancia solar: 148.181.308,81 km
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Today's Waxing Crescent Phase
The Waxing Crescent on November 8 has an illumination of 18%. This is the percentage of the Moon illuminated by the Sun. The illumination is constantly changing and can vary up to 10% a day. On November 8 the Moon is 4.14 days old.
The moon is close to the sun in the sky and mostly dark except for the right edge of the moon which becomes brighter as the days get closer to the next phase which is a First Quarter with a 50% illumination.
Phase Details For - November 8
Phase: Waxing Crescent
Illumination: 18%
Moon Age: 4.14 days
Moon Angle: 0.55
Moon Distance: 364,897.83 km
Sun Angle: 0.54
Sun Distance: 148,181,308.81 km
File:IMG_8395_Moon
El Mirador de la Memoria. 2
Statues dedicated to the Spanish civil war and Dictatorship forgotten. El Torno, Caceres, Extremadura, Spain.
Conjunto de estatuas dedicadas a los olvidados de la Guerra Civil y la Dictadura española, El Torno, Cáceres, Extremadura, España.
The Rosette Nebula (also known as NGC 2237 and C 49) is a large, roughly circular H II region located on the edge of a giant molecular nebula in the constellation Unicorn. The nebula has an angular diameter of 1.3° and is located at a distance of 1600 parsecs (about 5200 light years) from the solar system; it is approximately 100 light-years in size. At the center of the Rosette Nebula is a bright open cluster known as NGC 2244; the blue stars of the cluster, forming part of the OB association known as Monoceros OB2, emit ultraviolet radiation, which excites the gas of the nebula leading it to emit red light. The stellar wind from the O and B group of stars is thought to exert pressure on the interstellar cloud causing compression, followed by star formation; in fact, many Bok globules have been observed in the region, believed to be the site of star formation.
240 shots from my home stacked and processed with pipp + Autostakert! + Registax + Photoshop.
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240 fotos tomadas desde mi casa, apiladas y procesadas con PIPP + Autostakkert! + Registax + Photoshop.
The Sunflower Galaxy (also known as M 63 or NGC 5055) is a spiral galaxy visible in the Northern constellation of Hunting Dogs; it was discovered in 1779 by Pierre Méchain, colleague and friend of the Messier and who collaborated in the drafting of the famous catalog.
The Sunflower galaxy is a spiral of the Sb or Sc type, showing an irregular spiral design; apparently it appears to form a physical group with the Pinwheel Galaxy, the Vortex Galaxy and many other smaller galaxies; it could belong to the Group of M101 (subgroup of M51). The proper name sunflower is due to the very large number of spiral segments that surround the nucleus, well wrapped around it and pervaded by a large number of interstellar dust clouds; the total mass of the galaxy would be between 80 and 140 billion solar masses, with a diameter of 90,000 light years, which is similar to that of our Milky Way.
The distance is estimated at 37 million light years and moves away from us at a speed of 580 km / s. [1]
In May 1971, a type Ia supernova was observed between its arms, reaching apparent magnitude 11.8.
Distance from Earth: 27,000,000 light years
12 "Truss RC telescope reduced to 1790
Moravian off-axis guider and Moravian G0300 guide camera
Celestron 80/600 guide tube with Asi Zwo 224
Moravian G2 8300 camera with internal wheel
Ioptron Cem120 mount
Moonlite focuser and 3.5 "electronic rotator
Electronic temperature control and anti-condensation bands
Cls ccd, R, G, B, Ha 6nm filters, all Astronomik
Shooting data:
51x300s Cls Ccd
15x600s Ha 6nm
21x240s R
21x240s G
21x240s B
Processing: Pixinsight, Photoshop, star spikes, astronomy tools
Ngc 7023 IRIS
TS RC 12" Truss
Moravian G2 8300 mark II
Ioptron Cem120
Astronomik ccd cls 61 x 240s -20° bin2
Astronomik R 39 x 240s -20° bin2
Astronomik G 39 x 240s -20° bin2
Astronomik B 39 x 240s -20° bin2
Takahashi FSQ-106EDXIII
QSI 683 wsg-8
Astro-Physics Mach1AP GTO with GTOCP3
Astrodon L Tru-Balance E-Series Gen 2: 37 · 900s -30C bin 1x1
Astrodon R Tru-Balance E-Series Gen 2: 16 · 900s -30C bin 1x1
Astrodon G Tru-Balance E-Series Gen 2: 17 · 900s -30C bin 1x1
Astrodon B Tru-Balance E-Series Gen 2: 15 · 900s -30C bin 1x1
Pixinsight, Photoshop, star spikes, astronomy tools
Credit: Luca Dinoi and Roberto Colombari
Disfrutando de la astrofotografia junto a varios artistas del retrato de las luces...
www.instagram.com/felipe_cabellog/
#Galeriatakkheima
Desolación olvidada
El Mirador de la Memoria.
Statues dedicated to the Spanish civil war and Dictatorship forgotten. El Torno, Caceres, Extremadura, Spain.
Conjunto de estatuas dedicadas a los olvidados de la Guerra Civil y la Dictadura española, El Torno, Cáceres, Extremadura, España.
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California Nebula revisited: The California Nebula is an emission nebula located in the constellation Perseus. .
Astrografo Orion 254/1000 f3.9, ottiche Ultra con correzione 1/10 di lambda
Montatura Ioptron Cem120 guidata da celestron 80/600 e qhy5lM
Asi 294pro con rotatore e focheggiatore elettronico
Controllo elettronico fasce anticondensa
Software Sgp, pixinsight e photoshop
91 light da 180s gain 122 offset 30 0° filtro l-pro
61 light da 30s gain 122 offset 30 0° filtro l-pro
Happy Moonday!
Picture taken with my camera attached to a telescope at
Amparo Astronomical Center, last Saturday night.
Thanks a lot for your visits, comments, faves, invites, etc. Very much appreciated!
©All rights reserved. Do not use without my express consent. If you want to buy or use my pictures, please contact me at thelma.gatuzzo@gmail.com.
Image recorded remotely at DeepSkyWest with a Takahashi FSQ106EDXIII and a QSI 683WSG-8.
SII: 20x900s
Ha: 17x900s
OIII: 16x900s
Copyright: R. Colombari
________________________________
The prominent ridge of emission featured in this dramatic skyscape is cataloged as IC 5067. Part of a larger emission nebula with a distinctive shape, popularly called The Pelican Nebula, the ridge spans about 10 light-years following the curve of the cosmic pelican's head and neck. This false color view also translates the pervasive glow of narrow emission lines from atoms in the nebula to a color palette made popular in Hubble Space Telescope images of star forming regions. Fantastic, dark shapes inhabiting the 1/2 degree wide field are clouds of cool gas and dust sculpted by the winds and radiation from hot, massive stars. Close-ups of some of the sculpted clouds show clear signs of newly forming stars. The Pelican Nebula, itself cataloged as IC 5070, is about 2,000 light-years away. To find it, look northeast of bright star Deneb in the high flying constellation Cygnus.
Source: APOD NASA
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This pair of large, faint emission nebulae are located in the Constellation: Auriga : lies 12,000 light years away.
Imaging telescopes or lenses:
Vixen VSD
Imaging cameras: Starlight Express SXVR-H18
Mounts: Sky-Watcher MX
Guiding telescopes or lenses:Vixen VSD
Guiding cameras: sx loadstar
Software: Sequence Generator Pro, PHD, Photoshop CS5
At Sítio Macuquinho - Salesópolis - São Paulo.
Wishing everyone a Peaceful Travel Tuesday!
Thanks a lot for your visits, comments, faves, invites, etc. Very much appreciated!
© All my images are protected under international authors copyright laws and may not be downloaded, reproduced, copied, transmitted or manipulated by any means without my written explicit permission, including the use on websites and similar medias. All rights reserved. Please contact me at thelma.gatuzzo@gmail.com if you intend to buy or use any of my images.
My instagram if you like: @thelmag, @thelma_and_cats and @teg_photo_arts
Member of Nature’s Spirit
Good Stewards of Nature
La nebulosa Laguna (M8) , distante 4100 anni luce dalla Terra , è visibile anche ad occhio nudo . Le dimensioni della nebulosa sono di circa 110 anni luce ( un anno luce corrisponde a 9461 miliardi di chilometri) Dati di ripresa : Colori RGB , ripresi il 24 giugno 2017 , con una Reflex Canon 700d non modificata , e filtro UHC Optolong eos clip . Luminanza Halpha : realizzata in 8 serate tra agosto e settembre 2019 , con una Canon 1100d full spectrum e filtro Ha 12nm . Tutte le foto sono state fatte da casa mia , con un telescopio 200/1000 e montatura Neq6 pro . Esposizione totale : 13 ore
M 106 (also known as NGC 4258) is a spiral galaxy visible in the constellation of Hunting Dogs; it appears to contain a supermassive black hole inside.
M106 is an example of a Seyfert galaxy; the detection of unusual radio wave and X-ray emissions observed through the Very Large Baseline Array radio telescope indicates that probably part of the galaxy is precipitating into a supermassive black hole located in its center: in fact it seems that a mass equal to 36 million is contained in the core of solar masses, concentrated in a volume between 1/24 and 1/12 of a light year, or between 12,000 to 54,000 AU.
The shape of M106 resembles that of the Andromeda Galaxy (M31), but with a different inclination, so that all the structures of the dust clouds on the galactic plane are perfectly visible; the spiral arms are rich in H II regions which in the images are shown in blue and red color, depending on whether or not they are associated with clusters of particularly hot and bright stars. In 1981 a supernova appeared between its arms, classified as SN 1981K, which reached the sixteenth apparent magnitude; since the spectrum was not analyzed, it was never known what kind of supernova it was. The distance of the galaxy is estimated at 21-25 million light years and its total mass is approximately 190 billion solar masses; it moves away from us at the speed of 537 km / s.
12 "Truss RC telescope reduced to 1790
Moravian off-axis guider and Moravian G0300 guide camera
Celestron 80/600 guide tube with Asi Zwo 224
Moravian G2 8300 camera with internal wheel
Ioptron Cem120 mount
Moonlite focuser and 3.5 "electronic rotator
Electronic temperature control and anti-condensation bands
Cls ccd, R, G, B, Ha 6nm filters, all Astronomik
Shooting data:
51x240s Cls Ccd
15x600s HA
19x240s R
19x240s G
19x240s B
Processing: Pixinsight, Photoshop, star spikes, astronomy tools