https://blogsolar.space/2026/03/25/fin-de-la-era-espacial/2026-03-25T22:58:14+00:00monthlyhttps://blogsolar.space/historias-del-espacio/2026-03-22T16:51:57+00:00weekly0.6https://blogsolar.space/fin-de-la-era-espacial/https://blogsolar.space/wp-content/uploads/2026/03/image-2-2.pngimagehttps://blogsolar.space/wp-content/uploads/2026/03/image-2-3.pngimagehttps://blogsolar.space/wp-content/uploads/2026/03/image-2.pngimagehttps://blogsolar.space/wp-content/uploads/2026/03/image-2-1.pngimagehttps://blogsolar.space/wp-content/uploads/2026/03/image.jpegimagehttps://blogsolar.space/wp-content/uploads/2026/03/image-1.pngimagehttps://blogsolar.space/wp-content/uploads/2026/03/image.pngimage2026-03-22T16:51:49+00:00weekly0.6https://blogsolar.space/2026/02/26/lhs-1903e-un-autentico-mundo-al-reves/2026-02-27T00:02:16+00:00monthlyhttps://blogsolar.space/lhs-1903e-un-autentico-mundo-al-reves/https://blogsolar.space/wp-content/uploads/2026/02/image-4.pngimagehttps://blogsolar.space/wp-content/uploads/2026/02/image-2.pngimagehttps://blogsolar.space/wp-content/uploads/2026/02/image-3.pngimagehttps://blogsolar.space/wp-content/uploads/2026/02/image.jpegimage2026-02-26T23:51:52+00:00weekly0.6https://blogsolar.space/por-que-estamos-regresando-a-la-luna-y-por-que-tuvimos-que-espera-mas-de-50-anos-para-hacerlo/https://blogsolar.space/wp-content/uploads/2026/02/nasabudget.pngNASABudgethttps://blogsolar.space/wp-content/uploads/2026/02/image-1-1.pngimagehttps://blogsolar.space/wp-content/uploads/2026/02/image-1.pngimagehttps://blogsolar.space/wp-content/uploads/2026/02/image-1-2.pngimagehttps://blogsolar.space/wp-content/uploads/2026/02/image.pngimage2026-02-03T03:15:33+00:00weekly0.6https://blogsolar.space/2026/01/17/encuentros-cercanos-de-otro-tipo-cuando-te-visita-una-una-roca-espacial/2026-01-17T20:50:57+00:00monthlyhttps://blogsolar.space/encuentros-cercanos-de-otro-tipo-cuando-te-visita-una-una-roca-espacial/https://blogsolar.space/wp-content/uploads/2026/01/allendemeteorite.jpgAllendeMeteoritehttps://blogsolar.space/wp-content/uploads/2026/01/tunguska_ereignis-1.jpgTunguska_Ereignis-1https://blogsolar.space/wp-content/uploads/2026/01/ruthhamilton.jpgRuthHamiltonhttps://blogsolar.space/wp-content/uploads/2026/01/chelabynsk-1.pngChelabynskhttps://blogsolar.space/wp-content/uploads/2026/01/chelyabinsk_meteor_trace_15-02-2013.jpgChelyabinsk_meteor_trace_15-02-20132026-01-17T20:39:44+00:00weekly0.6https://blogsolar.space/2025/12/08/el-sol-esta-demasiado-frio-para-las-reacciones-nucleares-entonces-por-que-brilla/2025-12-08T14:02:12+00:00monthlyhttps://blogsolar.space/el-sol-esta-demasiado-frio-para-las-reacciones-nucleares-entonces-por-que-brilla/https://blogsolar.space/wp-content/uploads/2025/12/nightsky2.pngNightSky2https://blogsolar.space/wp-content/uploads/2025/12/solar-interior-eso.width-800.jpgsolar-interior-ESO.width-800https://blogsolar.space/wp-content/uploads/2025/12/image-2-1.pngimagehttps://blogsolar.space/wp-content/uploads/2025/12/image-3.pngimagehttps://blogsolar.space/wp-content/uploads/2025/12/image-3-1.pngimagehttps://blogsolar.space/wp-content/uploads/2025/12/image-3-2.pngimagehttps://blogsolar.space/wp-content/uploads/2025/12/image-2.pngimagehttps://blogsolar.space/wp-content/uploads/2025/12/image.pngimagehttps://blogsolar.space/wp-content/uploads/2025/12/image-1.pngimage2025-12-08T00:58:55+00:00weekly0.6https://blogsolar.space/2025/12/01/evento-del-clima-espacial/https://blogsolar.space/wp-content/uploads/2025/12/flare.pngFlarehttps://blogsolar.space/wp-content/uploads/2025/11/cme.pngCMEhttps://blogsolar.space/wp-content/uploads/2025/11/flare.pngFlare2025-12-01T06:14:37+00:00monthlyhttps://blogsolar.space/2025/11/30/nuevo/https://blogsolar.space/wp-content/uploads/2025/11/nuevo-1.pngNUevohttps://blogsolar.space/wp-content/uploads/2025/11/nuevo.pngNUevo2025-12-01T05:46:51+00:00monthlyhttps://blogsolar.space/bases-del-clima-espacial/2025-11-21T03:11:34+00:00weekly0.6https://blogsolar.space/2537-2/https://blogsolar.space/wp-content/uploads/2025/11/title-alert-esp-1.pngTitle-Alert-ESPhttps://blogsolar.space/wp-content/uploads/2025/11/rafagas-clasificacion-esp.pngRafagas-Clasificacion-ESPhttps://blogsolar.space/wp-content/uploads/2025/11/title-alert-esp.pngTitle-Alert-ESPhttps://blogsolar.space/wp-content/uploads/2025/11/x_class_solar_flare_sends_e28098shockwaves_on_the_sun_6819094556.jpgX Class Solar Flare Sends ‘Shockwaves’ on The SunNASA image captured March 6, 2012
To view a video of this event go to: <a href="http://www.flickr.com/photos/gsfc/6815861366">www.flickr.com/photos/gsfc/6815861366</a>
The sun erupted with one of the largest solar flares of this solar cycle on March 6, 2012 at 7PM ET. This flare was categorized as an X5.4, making it the second largest flare -- after an X6.9 on August 9, 2011 -- since the sun’s activity segued into a period of relatively low activity called solar minimum in early 2007. The current increase in the number of X-class flares is part of the sun’s normal 11-year solar cycle, during which activity on the sun ramps up to solar maximum, which is expected to peak in late 2013.
About an hour later, at 8:14 PM ET, March 6, the same region let loose an X1.3 class flare. An X1 is 5 times smaller than an X5 flare.
These X-class flares erupted from an active region named AR 1429 that rotated into view on March 2. Prior to this, the region had already produced numerous M-class and one X-class flare. The region continues to rotate across the front of the sun, so the March 6 flare was more Earthward facing than the previous ones. It triggered a temporary radio blackout on the sunlit side of Earth that interfered with radio navigation and short wave radio.
In association with these flares, the sun also expelled two significant coronal mass ejections (CMEs), which are travelling faster than 600 miles a second and may arrive at Earth in the next few days. In the meantime, the CME associated with the X-class flare from March 4 has dumped solar particles and magnetic fields into Earth’s atmosphere and distorted Earth's magnetic fields, causing a moderate geomagnetic storm, rated a G2 on a scale from G1 to G5. Such storms happen when the magnetic fields around Earth rapidly change strength and shape. A moderate storm usually causes aurora and may interfere with high frequency radio transmission near the poles. This storm is already dwindling, but the Earth may experience another enhancement if the most recent CMEs are directed toward and impact Earth.
In addition, last night’s flares have sent solar particles into Earth’s atmosphere, producing a moderate solar energetic particle event, also called a solar radiation storm. These particles have been detected by NASA’s SOHO and STEREO spacecraft, and NOAA’s GOES spacecraft. At the time of writing, this storm is rated an S3 on a scale that goes up to S5. Such storms can interfere with high frequency radio communication.
Besides the August 2011 X-class flare, the last time the sun sent out flares of this magnitude was in 2006. There was an X6.5 on December 6, 2006 and an X9.0 on December 5, 2006. Like the most recent events, those two flares erupted from the same region on the sun, which is a common occurrence.
Credit: NASA/SDO/AIA
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Starshot2025-11-03T18:52:33+00:00weekly0.6https://blogsolar.space/retrasos-aereos-y-riesgo-para-la-salud-el-impacto-del-clima-espacial/https://blogsolar.space/wp-content/uploads/2025/09/jet_stream_print_res.jpgjet_stream_print_reshttps://blogsolar.space/wp-content/uploads/2025/09/iaea_doses.pngIAEA_doseshttps://blogsolar.space/wp-content/uploads/2025/09/tobiska16.jpgTobiska16https://blogsolar.space/wp-content/uploads/2025/09/ionospheric_reflectionesp.pngIonospheric_reflectionESPhttps://blogsolar.space/wp-content/uploads/2025/09/1280px-sun_-_august_1_2010.jpg1280px-Sun_-_August_1,_2010https://blogsolar.space/wp-content/uploads/2025/09/cx831.pngCX8312025-09-24T13:31:51+00:00weekly0.6https://blogsolar.space/mayor-vulnerabilidad-de-los-satelites-durante-tormentas-solares-debido-a-la-creciente-concentracion-de-co%e2%82%82/https://blogsolar.space/wp-content/uploads/2025/09/earth_s_atmosphereesp.pngEarth_s_atmosphereESPhttps://blogsolar.space/wp-content/uploads/2025/09/starlink_mission_47926144123.jpgStarlink_Mission_(47926144123)2025-09-09T19:07:24+00:00weekly0.6https://blogsolar.space/una-doble-explosion-de-supernova-que-destruyo-las-teorias-sobre-supernovas/https://blogsolar.space/wp-content/uploads/2025/07/accretion_disk_binary_system.jpgAccretion_Disk_Binary_Systemhttps://blogsolar.space/wp-content/uploads/2025/07/witharrows.jpgWithArrows2025-07-10T23:09:30+00:00weekly0.6https://blogsolar.space/ocurrio-lo-impensable-recortes-a-la-ciencia-sin-precedentes/https://blogsolar.space/wp-content/uploads/2025/07/artemis_phase_1.jpgArtemis_Phase_1https://blogsolar.space/wp-content/uploads/2025/07/nasa_budget_historical_inflation_adjusted_fy2026_threat_desktop.pngnasa_budget_historical_inflation_adjusted_fy2026_threat_desktop2025-07-04T04:03:40+00:00weekly0.6https://blogsolar.space/2025/07/03/ocurrio-lo-impensable-recortes-a-la-ciencia-sin-precedentes/2025-07-04T04:03:07+00:00monthlyhttps://blogsolar.space/noticias-del-espacio/2025-07-03T22:50:01+00:00weekly0.6https://blogsolar.space/2025/06/29/nuevo-en-el-blog-solar/2025-06-29T20:09:15+00:00monthlyhttps://blogsolar.space/calendario-astronomico/2025-06-29T19:49:07+00:00weekly0.6https://blogsolar.space/2025/06/27/que-tan-altas-son-las-montanas-en-los-pulsares/https://blogsolar.space/wp-content/uploads/2025/06/pulsar_schematic.svg_-2.pngPulsar_schematic.svghttps://blogsolar.space/wp-content/uploads/2025/06/vela_pulsar_jet.jpgVela_Pulsar_jethttps://blogsolar.space/wp-content/uploads/2025/06/pulsar_schematic.svg_-1.pngPulsar_schematic.svg2025-06-28T16:43:23+00:00monthlyhttps://blogsolar.space/que-tan-altas-son-las-montanas-en-los-pulsares/https://blogsolar.space/wp-content/uploads/2025/06/lightsmall-optimised.gifLightsmall-optimisedhttps://blogsolar.space/wp-content/uploads/2025/06/pulsar_schematic.svg_.pngPulsar_schematic.svghttps://blogsolar.space/wp-content/uploads/2025/06/white_dwarf_vs_neutron_star.svg_.pngWhite_dwarf_vs_neutron_star.svg2025-06-27T19:24:27+00:00weekly0.6https://blogsolar.space/2025/06/22/asi-fue-la-capsula-promocional-para-el-programa-de-once-lab-del-canal-once/2025-06-22T19:49:59+00:00monthlyhttps://blogsolar.space/2025/06/22/colaboramos-con-canal-11-en-el-tema-del-clima-espacial/2025-06-22T19:45:07+00:00monthlyhttps://blogsolar.space/2025/06/20/revelan-imagenes-ineditas-del-polo-sur-del-sol/2025-06-20T17:27:48+00:00monthlyhttps://blogsolar.space/revelan-imagenes-ineditas-del-polo-sur-del-sol/https://blogsolar.space/wp-content/uploads/2025/06/spice.pngSpicehttps://blogsolar.space/wp-content/uploads/2025/06/phi_s_pole-to-pole_view_of_the_sun_s_magnetic_field_pillars.gifPHI_s_pole-to-pole_view_of_the_Sun_s_magnetic_field_pillars2025-06-20T17:03:39+00:00weekly0.6https://blogsolar.space/megaexplosiones-cosmicas-que-desconciertan-a-los-astronomos/https://blogsolar.space/wp-content/uploads/2025/06/nasa.jpgNASA2025-06-12T23:26:15+00:00weekly0.6https://blogsolar.space/2025/06/12/megaexplosiones-cosmicas-que-desconciertan-a-los-astronomos/2025-06-12T23:22:47+00:00monthlyhttps://blogsolar.space/2025/05/31/james-webb-posiblemente-descubrio-un-monstruo-oculto-en-la-galaxia-m83/https://blogsolar.space/wp-content/uploads/2025/05/weic2509a-1.jpgM83 (MIRI image)The barred spiral galaxy Messier 83 (M83) is featured in detail in this image from the NASA/ESA/CSA James Webb Space Telescope. M83, which is also known as NGC 5236, was observed for this image with the Mid-Infrared Instrument (MIRI). Now, further data from MIRI has enabled a new discovery in M83. Astronomers using Webb have discovered evidence that suggests the presence of a long-sought supermassive black hole at the heart of the nearby spiral galaxy M83. This surprising finding, made possible by Webb’s MIRI, reveals highly ionised neon gas that could be a telltale signature of an active galactic nucleus (AGN), a growing black hole at the center of a galaxy. This image was compiled using data collected through just two of MIRI’s ten filters, near the short end of the instrument’s wavelength range. The result is this extraordinarily detailed image, with its creeping tendrils of gas, dust and stars. In this image, the bright blue shows the distribution of stars across the central part of the galaxy. The bright yellow regions that weave through the spiral arms indicate concentrations of active stellar nurseries, where new stars are forming. The orange-red areas indicate the distribution of a type of carbon-based compound known as polycyclic aromatic hydrocarbons (or PAHs) — the F770W filter, one of the two used here, is particularly suited to imaging these important molecules. The data for this image come from a series of observations collectively titled Feedback in Emerging extrAgalactic Star clusTers, or FEAST. [Image Description: A close-up view of a barred spiral galaxy. Two spiral arms reach horizontally away from the core in the centre, merging into a broad network of gas and dust which fills the image. This material glows brightest orange along the path of the arms, and is darker red across the rest of the galaxy. Through many gaps in the dust, countless tiny stars can be seen, most densely around the core.]2025-06-01T17:03:22+00:00monthlyhttps://blogsolar.space/james-webb-posiblemente-descubrio-un-monstruo-oculto-en-la-galaxia-m83/https://blogsolar.space/wp-content/uploads/2025/05/centairusa.jpgCentaurus AColour composite image of Centaurus A, revealing the lobes and jets emanating from the active galaxy’s central black hole. This is a composite of images obtained with three instruments, operating at very different wavelengths. The 870-micron submillimetre data, from LABOCA on APEX, are shown in orange. X-ray data from the Chandra X-ray Observatory are shown in blue. Visible light data from the Wide Field Imager (WFI) on the MPG/ESO 2.2 m telescope located at La Silla, Chile, show the stars and the galaxy’s characteristic dust lane in close to "true colour". #Lhttps://blogsolar.space/wp-content/uploads/2025/05/saga.pngSagAhttps://blogsolar.space/wp-content/uploads/2025/05/weic2509a.jpgM83 (MIRI image)The barred spiral galaxy Messier 83 (M83) is featured in detail in this image from the NASA/ESA/CSA James Webb Space Telescope. M83, which is also known as NGC 5236, was observed for this image with the Mid-Infrared Instrument (MIRI). Now, further data from MIRI has enabled a new discovery in M83. Astronomers using Webb have discovered evidence that suggests the presence of a long-sought supermassive black hole at the heart of the nearby spiral galaxy M83. 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The data for this image come from a series of observations collectively titled Feedback in Emerging extrAgalactic Star clusTers, or FEAST. [Image Description: A close-up view of a barred spiral galaxy. Two spiral arms reach horizontally away from the core in the centre, merging into a broad network of gas and dust which fills the image. This material glows brightest orange along the path of the arms, and is darker red across the rest of the galaxy. Through many gaps in the dust, countless tiny stars can be seen, most densely around the core.]2025-05-31T22:43:42+00:00weekly0.6https://blogsolar.space/2025/05/22/2334/https://blogsolar.space/wp-content/uploads/2025/05/aurorasjupiter-1.webpAurorasJupiter2025-05-22T18:38:00+00:00monthlyhttps://blogsolar.space/misteriosas-auroras-bailantes-en-jupiter-reveladas-por-webb/https://blogsolar.space/wp-content/uploads/2025/05/aurorasjupiter.webpAurorasJupiter2025-05-21T19:51:18+00:00weekly0.6https://blogsolar.space/2025/05/16/2325/2025-05-16T20:16:16+00:00monthlyhttps://blogsolar.space/los-arboles-que-anticiparon-el-eclipse/https://blogsolar.space/wp-content/uploads/2025/05/senzorji.pngSenzorjihttps://blogsolar.space/wp-content/uploads/2025/05/eclipse22.pngEclipse222025-05-16T18:20:33+00:00weekly0.6https://blogsolar.space/2025/05/08/2316/2025-05-08T22:43:14+00:00monthlyhttps://blogsolar.space/quien-sera-el-dueno-del-espacio-la-nueva-carrera-armamentista-y-la-lucha-por-la-ultima-frontera/https://blogsolar.space/wp-content/uploads/2025/05/posta_romana_-_1959_-_laika_120_b.jpgPosta_Romana_-_1959_-_Laika_120_Bhttps://blogsolar.space/wp-content/uploads/2025/05/sputnik_asm.jpgSputnik_asmCamera: DCS420A
Serial #: 420-2040
Width: 1524
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Date: 11/24/97
Time: 11:39:45
DCS4XX Image
FW Ver: 081596
TIFF Image
Look: Product
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Counter: [88]
ISO: 100
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Flash sync: Norm
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Focus area: Wide
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Space Launch System rocket carrying the Orion spacecraft launches on the Artemis I flight test, Wednesday, Nov. 16, 2022, from Launch Complex 39B at NASA’s Kennedy Space Center in Florida. NASA’s Artemis I mission is the first integrated flight test of the agency’s deep space exploration systems: the Orion spacecraft, Space Launch System (SLS) rocket, and ground systems. SLS and Orion launched at 1:47 a.m. EST, from Launch Pad 39B at the Kennedy Space Center. Photo Credit: (NASA/Joel Kowsky)https://blogsolar.space/wp-content/uploads/2023/10/ariane6.pngariane62023-10-19T16:08:02+00:00weekly0.6https://blogsolar.space/2023/10/19/https-blogsolar-space-al-marte-con-cohetes-nucleares/https://blogsolar.space/wp-content/uploads/2023/10/banneresp.jpgbanneresp2023-10-19T16:06:58+00:00monthlyhttps://blogsolar.space/2023/09/30/1712/https://blogsolar.space/wp-content/uploads/2023/09/predavanja2023todos.pngpredavanja2023todos2023-10-19T16:04:57+00:00monthlyhttps://blogsolar.space/2023/09/20/1709/https://blogsolar.space/wp-content/uploads/2023/09/taller-eclipse-27-sep_eclipse-2.jpgtaller-eclipse-27-sep_eclipse-22023-09-20T14:02:31+00:00monthlyhttps://blogsolar.space/2023/09/10/1697/https://blogsolar.space/wp-content/uploads/2023/09/origendelsol.pngorigendelsolhttps://blogsolar.space/wp-content/uploads/2023/09/izvorsonca.pngizvorsonca2023-09-10T20:23:06+00:00monthlyhttps://blogsolar.space/somos-de-la-misma-sustancia-que-las-estrellas/https://blogsolar.space/wp-content/uploads/2023/09/allende_meteorite.jpgallende_meteoritehttps://blogsolar.space/wp-content/uploads/2023/09/orion_nebula_-_hubble_2006_mosaic_18000-1.jpgorion_nebula_-_hubble_2006_mosaic_18000-1This dramatic image offers a peek inside a cavern of roiling dust and gas where thousands of stars are forming. The image, taken by the Advanced Camera for Surveys (ACS) aboard NASA/ESA Hubble Space Telescope, represents the sharpest view ever taken of this region, called the Orion Nebula. More than 3,000 stars of various sizes appear in this image. Some of them have never been seen in visible light. These stars reside in a dramatic dust-and-gas landscape of plateaus, mountains, and valleys that are reminiscent of the Grand Canyon. The Orion Nebula is a picture book of star formation, from the massive, young stars that are shaping the nebula to the pillars of dense gas that may be the homes of budding stars. The bright central region is the home of the four heftiest stars in the nebula. The stars are called the Trapezium because they are arranged in a trapezoid pattern. Ultraviolet light unleashed by these stars is carving a cavity in the nebula and disrupting the growth of hundreds of smaller stars. Located near the Trapezium stars are stars still young enough to have disks of material encircling them. These disks are called protoplanetary disks or "proplyds" and are too small to see clearly in this image. The disks are the building blocks of solar systems. The bright glow at upper left is from M43, a small region being shaped by a massive, young star's ultraviolet light. Astronomers call the region a miniature Orion Nebula because only one star is sculpting the landscape. The Orion Nebula has four such stars. Next to M43 are dense, dark pillars of dust and gas that point toward the Trapezium. These pillars are resisting erosion from the Trapezium's intense ultraviolet light. The glowing region on the right reveals arcs and bubbles formed when stellar winds - streams of charged particles ejected from the Trapezium stars - collide with material. The faint red stars near the bottom are the myriad brown dwarfs that Hubble spied for the first time in the nebula in visible light. Sometimes called "failed stars," brown dwarfs are cool objects that are too small to be ordinary stars because they cannot sustain nuclear fusion in their cores the way our Sun does. The dark red column, below, left, shows an illuminated edge of the cavity wall. The Orion Nebula is 1,500 light-years away, the nearest star-forming region to Earth. Astronomers used 520 Hubble images, taken in five colours, to make this picture. They also added ground-based photos to fill out the nebula. The ACS mosaic covers approximately the apparent angular size of the full moon. The Orion observations were taken between 2004 and 2005.https://blogsolar.space/wp-content/uploads/2023/09/orion_nebula_-_hubble_2006_mosaic_18000.jpgorion_nebula_-_hubble_2006_mosaic_18000This dramatic image offers a peek inside a cavern of roiling dust and gas where thousands of stars are forming. The image, taken by the Advanced Camera for Surveys (ACS) aboard NASA/ESA Hubble Space Telescope, represents the sharpest view ever taken of this region, called the Orion Nebula. More than 3,000 stars of various sizes appear in this image. Some of them have never been seen in visible light. These stars reside in a dramatic dust-and-gas landscape of plateaus, mountains, and valleys that are reminiscent of the Grand Canyon. The Orion Nebula is a picture book of star formation, from the massive, young stars that are shaping the nebula to the pillars of dense gas that may be the homes of budding stars. The bright central region is the home of the four heftiest stars in the nebula. The stars are called the Trapezium because they are arranged in a trapezoid pattern. Ultraviolet light unleashed by these stars is carving a cavity in the nebula and disrupting the growth of hundreds of smaller stars. Located near the Trapezium stars are stars still young enough to have disks of material encircling them. These disks are called protoplanetary disks or "proplyds" and are too small to see clearly in this image. The disks are the building blocks of solar systems. The bright glow at upper left is from M43, a small region being shaped by a massive, young star's ultraviolet light. Astronomers call the region a miniature Orion Nebula because only one star is sculpting the landscape. The Orion Nebula has four such stars. Next to M43 are dense, dark pillars of dust and gas that point toward the Trapezium. These pillars are resisting erosion from the Trapezium's intense ultraviolet light. The glowing region on the right reveals arcs and bubbles formed when stellar winds - streams of charged particles ejected from the Trapezium stars - collide with material. The faint red stars near the bottom are the myriad brown dwarfs that Hubble spied for the first time in the nebula in visible light. Sometimes called "failed stars," brown dwarfs are cool objects that are too small to be ordinary stars because they cannot sustain nuclear fusion in their cores the way our Sun does. The dark red column, below, left, shows an illuminated edge of the cavity wall. The Orion Nebula is 1,500 light-years away, the nearest star-forming region to Earth. Astronomers used 520 Hubble images, taken in five colours, to make this picture. They also added ground-based photos to fill out the nebula. The ACS mosaic covers approximately the apparent angular size of the full moon. The Orion observations were taken between 2004 and 2005.https://blogsolar.space/wp-content/uploads/2023/09/barnard_68.jpgbarnard_682023-09-10T20:10:45+00:00weekly0.6https://blogsolar.space/2023/08/04/1619/https://blogsolar.space/wp-content/uploads/2023/07/sobradelsol.pngsobradelsolhttps://blogsolar.space/wp-content/uploads/2023/06/fig1-2.pngfig1-22023-08-06T10:57:00+00:00monthlyhttps://blogsolar.space/la-sombra-del-sol/https://blogsolar.space/wp-content/uploads/2023/06/sombradelsolciclosolar.pngsombradelsolciclosolarhttps://blogsolar.space/wp-content/uploads/2023/06/fig1-1.pngfig1-1https://blogsolar.space/wp-content/uploads/2023/06/fig1.pngfig1https://blogsolar.space/wp-content/uploads/2023/06/fig4.pngfig4https://blogsolar.space/wp-content/uploads/2023/06/fig5.pngfig5https://blogsolar.space/wp-content/uploads/2023/06/fig3.pngfig3https://blogsolar.space/wp-content/uploads/2023/06/fig2-1.pngfig2-1https://blogsolar.space/wp-content/uploads/2023/06/fig2.pngfig22023-08-06T10:56:38+00:00weekly0.6https://blogsolar.space/2023/07/04/1630/https://blogsolar.space/wp-content/uploads/2023/06/fig1-1.jpgfig1-12023-07-04T19:57:29+00:00monthlyhttps://blogsolar.space/2023/06/08/1600/2023-06-09T01:17:38+00:00monthlyhttps://blogsolar.space/2023/05/30/1575/2023-05-30T22:40:31+00:00monthlyhttps://blogsolar.space/2023/05/24/1558/https://blogsolar.space/wp-content/uploads/2023/05/image-1.pngimage-1https://blogsolar.space/wp-content/uploads/2023/05/image.pngimagehttps://blogsolar.space/wp-content/uploads/2023/05/movie.gifmovie2023-05-25T04:47:47+00:00monthlyhttps://blogsolar.space/2023/05/16/1552/https://blogsolar.space/wp-content/uploads/2023/05/vodanaluniespbanner.pngvodanaluniespbanner2023-05-17T05:47:45+00:00monthlyhttps://blogsolar.space/abunda-el-agua-en-la-luna/https://blogsolar.space/wp-content/uploads/2023/05/chang-e-5-assembly-cg-1-cropped.jpgchang-e-5-assembly-cg-1-croppedhttps://blogsolar.space/wp-content/uploads/2023/05/langrenus_map_of_the_moon_1645.jpglangrenus_map_of_the_moon_1645https://blogsolar.space/wp-content/uploads/2023/05/fullmoon2010.jpgfullmoon20102023-05-17T05:44:14+00:00weekly0.6https://blogsolar.space/imagenes-viejas-revelan-volcan-activo-en-venus/https://blogsolar.space/wp-content/uploads/2023/05/venus-surface-venera-14-camera-2-1982.jpgvenus-surface-venera-14-camera-2-1982https://blogsolar.space/wp-content/uploads/2023/05/venusearthsize-nasa-apollo-17.jpgvenusearthsize-nasa-apollo-17https://blogsolar.space/wp-content/uploads/2023/05/venus-surface-magellan-4-nasa.jpgvenus-surface-magellan-4-nasa2023-05-03T22:17:57+00:00weekly0.6https://blogsolar.space/2023/05/03/1512/https://blogsolar.space/wp-content/uploads/2023/05/venusesp.pngvenusesp2023-05-03T21:54:15+00:00monthlyhttps://blogsolar.space/nieve-espacial-en-una-luna-saturno/https://blogsolar.space/wp-content/uploads/2023/03/saturn-by-cassini-nasa.jpgsaturn-by-cassini-nasahttps://blogsolar.space/wp-content/uploads/2023/03/enceladus_plumes-nasajplspace-science-institute.jpgconverted PNM fileconverted PNM filehttps://blogsolar.space/wp-content/uploads/2023/03/enceladus_interior_pillars-esa-non-annotated.jpgenceladus_interior_pillars-esa-non-annotatedhttps://blogsolar.space/wp-content/uploads/2023/03/tigerstripes-cassini-imaging-team-ssi-jpl-esa-nasa.jpgtigerstripes-cassini-imaging-team-ssi-jpl-esa-nasa2023-05-03T19:54:21+00:00weekly0.6https://blogsolar.space/2023/04/12/1493/2023-04-12T15:21:04+00:00monthlyhttps://blogsolar.space/2023/04/09/1467/2023-04-10T04:17:36+00:00monthlyhttps://blogsolar.space/glosario/2023-04-10T03:32:03+00:00weekly0.6https://blogsolar.space/2023/04/03/1461/https://blogsolar.space/wp-content/uploads/2023/04/artemis-1-a.jpgArtemis I First RolloutNASA’s Space Launch System (SLS) rocket with the Orion spacecraft aboard is seen atop a mobile launcher as it rolls out of High Bay 3 of the Vehicle Assembly Building for the first time to Launch Complex 39B, Thursday, March 17, 2022, at NASA’s Kennedy Space Center in Florida. Ahead of NASA’s Artemis I flight test, the fully stacked and integrated SLS rocket and Orion spacecraft will undergo a wet dress rehearsal at Launch Complex 39B to verify systems and practice countdown procedures for the first launch. 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TIFF fileIDL TIFF filehttps://blogsolar.space/wp-content/uploads/2023/01/saturns_ring_plane-nasa-jpl-space-science-institute.svg_-1.pngsaturns_ring_plane-nasa-jpl-space-science-institute.svg_-1https://blogsolar.space/wp-content/uploads/2023/01/saturns_ring_plane-nasa-jpl-space-science-institute.svg_.pngsaturns_ring_plane-nasa-jpl-space-science-institute.svg_https://blogsolar.space/wp-content/uploads/2023/01/huygens_systema_saturnium.jpghuygens_systema_saturnium2023-03-07T22:06:45+00:00weekly0.6https://blogsolar.space/programa-artemis-el-gran-regreso-de-la-humanidad-a-la-luna/https://blogsolar.space/wp-content/uploads/2023/01/lunar_electric_rover-nasa-regan-geeseman.jpglunar_electric_rover-nasa-regan-geesemanhttps://blogsolar.space/wp-content/uploads/2023/01/moon-base-2-nasa.jpgmoon-base-2-nasahttps://blogsolar.space/wp-content/uploads/2023/01/sls-nasa-joel-kowsky.jpgArtemis I PreflightNASA’s Space Launch System (SLS) rocket with the Orion spacecraft aboard is seen atop a mobile launcher at Launch Pad 39B, Thursday, Aug. 18, 2022, after being rolled out to the launch pad at NASA’s Kennedy Space Center in Florida. NASA’s Artemis I mission is the first integrated test of the agency’s deep space exploration systems: the Orion spacecraft, SLS rocket, and supporting ground systems. Launch of the uncrewed flight test is targeted for no earlier than Aug. 29. Photo Credit: (NASA/Joel Kowsky)2023-03-07T22:06:38+00:00weekly0.6https://blogsolar.space/breve-historia-de-los-ciclos-solares/https://blogsolar.space/wp-content/uploads/2023/01/screen-shot-2021-07-17-at-22.37.34.pngscreen-shot-2021-07-17-at-22.37.34https://blogsolar.space/wp-content/uploads/2023/01/screen-shot-2021-07-17-at-22.37.27.pngscreen-shot-2021-07-17-at-22.37.27https://blogsolar.space/wp-content/uploads/2023/01/screen-shot-2021-07-17-at-22.37.17.pngscreen-shot-2021-07-17-at-22.37.172023-03-07T22:06:03+00:00weekly0.6https://blogsolar.space/clima-del-espacio/https://blogsolar.space/wp-content/uploads/2023/01/newspapers2.jpgnewspapers2https://blogsolar.space/wp-content/uploads/2023/01/carrington_richard_sunspots_1859.jpgcarrington_richard_sunspots_1859https://blogsolar.space/wp-content/uploads/2023/01/richard-carrington.jpgrichard-carrington2023-03-07T22:06:00+00:00weekly0.6https://blogsolar.space/el-desastre-que-creo-la-luna/https://blogsolar.space/wp-content/uploads/2023/01/lunadesastre.pnglunadesastrehttps://blogsolar.space/wp-content/uploads/2023/01/fullmoon2010.jpgfullmoon20102023-03-07T22:05:56+00:00weekly0.6https://blogsolar.space/el-dia-que-desaparecio-el-viento-solar/https://blogsolar.space/wp-content/uploads/2023/01/nasa-polar-aurorae.jpgnasa-polar-aurorae2023-03-07T22:05:52+00:00weekly0.6https://blogsolar.space/asi-fue-como-descubrimos-el-viento-solar/https://blogsolar.space/wp-content/uploads/2023/01/nasajet-propulsion-laboratory.jpgnasajet-propulsion-laboratoryhttps://blogsolar.space/wp-content/uploads/2023/01/nasa-aurorae.jpgnasa-auroraehttps://blogsolar.space/wp-content/uploads/2023/01/by-richard-carrington.jpgby-richard-carrington2023-03-07T22:05:48+00:00weekly0.6https://blogsolar.space/la-mision-que-buscara-gas-natural-en-titan/https://blogsolar.space/wp-content/uploads/2023/01/dragonfly-on-surface.jpgdragonfly-on-surfacehttps://blogsolar.space/wp-content/uploads/2023/01/682400main_pia14922_full_full.jpg682400main_pia14922_full_full2023-03-07T22:05:43+00:00weekly0.6https://blogsolar.space/el-gran-problema-de-los-viajes-espaciales/https://blogsolar.space/wp-content/uploads/2023/01/screen-shot-2021-07-17-at-21.58.41.pngscreen-shot-2021-07-17-at-21.58.41https://blogsolar.space/wp-content/uploads/2023/01/screen-shot-2021-07-17-at-21.58.31.pngscreen-shot-2021-07-17-at-21.58.31https://blogsolar.space/wp-content/uploads/2023/01/screen-shot-2021-07-17-at-21.58.21.pngscreen-shot-2021-07-17-at-21.58.212023-03-07T22:05:39+00:00weekly0.6https://blogsolar.space/la-sustancia-mas-antigua-en-la-tierra/https://blogsolar.space/wp-content/uploads/2023/01/murchison-basilicofresc-wikimedia-commons.jpgmurchison-basilicofresc-wikimedia-commonshttps://blogsolar.space/wp-content/uploads/2023/01/allende-andersen-and-haack-2005-3.jpgallende-andersen-and-haack-2005-32023-03-07T22:05:34+00:00weekly0.6https://blogsolar.space/las-fogatas-solares/https://blogsolar.space/wp-content/uploads/2023/01/chen21.gifchen21https://blogsolar.space/wp-content/uploads/2023/01/esa-solar-orbiter.jpgesa-solar-orbiter2023-03-07T22:05:30+00:00weekly0.6https://blogsolar.space/moleculas-organicas-en-marte/https://blogsolar.space/wp-content/uploads/2023/01/nasa-2-gale.jpgnasa-2-galehttps://blogsolar.space/wp-content/uploads/2023/01/nasa-jpl-caltech-msss-curiosity.jpgUpdated Curiosity Self-Portrait at 'John Klein'Updated Curiosity Self-Portrait at 'John Klein'2023-03-07T22:05:05+00:00weekly0.6https://blogsolar.space/mundos-lejanos-donde-llueven-los-diamantes/https://blogsolar.space/wp-content/uploads/2023/01/neptune_clouds-nasa-jpl.jpgneptune_clouds-nasa-jplhttps://blogsolar.space/wp-content/uploads/2023/01/neptunes_great_dark_spot-nasa-jpl.jpgneptunes_great_dark_spot-nasa-jplhttps://blogsolar.space/wp-content/uploads/2023/01/uranus-neptune-nasa.jpguranus-neptune-nasaNASA???s Voyager 2 spacecraft captured these views of Uranus (on the left) and Neptune (on the right) during its flybys of the planets in the 1980s.2023-03-07T22:05:00+00:00weekly0.6https://blogsolar.space/la-razon-de-los-diferentes-colores-de-urano-y-neptuno/https://blogsolar.space/wp-content/uploads/2023/01/nasa.jpgnasahttps://blogsolar.space/wp-content/uploads/2023/01/uranus-neptune-nasa-1.jpguranus-neptune-nasa-1NASA???s Voyager 2 spacecraft captured these views of Uranus (on the left) and Neptune (on the right) during its flybys of the planets in the 1980s.2023-03-07T22:04:53+00:00weekly0.6https://blogsolar.space/no-miren-hacia-arriba/https://blogsolar.space/wp-content/uploads/2023/01/lunar_landscapes-nasa-gsfc-arizona-state-university.jpglunar_landscapes-nasa-gsfc-arizona-state-universityLunar Landscapes - On a few occasions the LRO team has taken the opportunity to tilt the spacecraft to a steep angle and use the LRO Narrow Angle Cameras to gather oblique images like this one. By looking across the landscape rather than straight down, topography and lighting angles are emphasized, giving a dramatic view of the lunar terrain. The northern plains region of the moon shown here has not been well studied and has few named features. The full size of this panorama is over 280 million pixels and it can be zoomed in on and explored more fully at the Lunar Reconnaissance Orbiter Camera’s web site.
Credit: NASA/GSFC/ASU
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