A small tool to view real-world ActivityPub objects as JSON! Enter a URL
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to the server to view the underlying object.
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"content": "<a href=\"https://www.minds.com/search?f=top&t=all&q=UMPlus\" title=\"#UMPlus\" class=\"u-url hashtag\" target=\"_blank\">#UMPlus</a> - Propeller Nebula by David Lindemann<br /><br /><a href=\"https://www.universomagico.net/2025/06/nebulosa-propulsor-por-david-lindemann.html\" target=\"_blank\">https://www.universomagico.net/2025/06/nebulosa-propulsor-por-david-lindemann.html</a><br /><br /><a href=\"https://www.minds.com/groups/profile/1144295236524617728/feed\" target=\"_blank\">https://www.minds.com/groups/profile/1144295236524617728/feed</a><br /><br />This spectacular image by astronomer David Lindemann primarily shows a striking cloud called the Propeller Nebula. It is also cataloged as Simeis 57 and has four designations in the DWB catalog based on its parts. The image displays a large amount of hydrogen, which is ionized by nearby hot, young stars. The Propeller Nebula is only a few tens of times the mass of the Sun. Its low mass and the fact that its distance has not been measured give it the status of a mysterious and enigmatic object. Located in the direction of the constellation.....<br /><a href=\"https://www.minds.com/search?f=top&t=all&q=astronomy\" title=\"#astronomy\" class=\"u-url hashtag\" target=\"_blank\">#astronomy</a> <a href=\"https://www.minds.com/search?f=top&t=all&q=space\" title=\"#space\" class=\"u-url hashtag\" target=\"_blank\">#space</a> <a href=\"https://www.minds.com/search?f=top&t=all&q=astrophysics\" title=\"#astrophysics\" class=\"u-url hashtag\" target=\"_blank\">#astrophysics</a> <a href=\"https://www.minds.com/search?f=top&t=all&q=astrophotography\" title=\"#astrophotography\" class=\"u-url hashtag\" target=\"_blank\">#astrophotography</a> ",
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"content": "#UMPlus - Propeller Nebula by David Lindemann\n\nhttps://www.universomagico.net/2025/06/nebulosa-propulsor-por-david-lindemann.html\n\nhttps://www.minds.com/groups/profile/1144295236524617728/feed\n\nThis spectacular image by astronomer David Lindemann primarily shows a striking cloud called the Propeller Nebula. It is also cataloged as Simeis 57 and has four designations in the DWB catalog based on its parts. The image displays a large amount of hydrogen, which is ionized by nearby hot, young stars. The Propeller Nebula is only a few tens of times the mass of the Sun. Its low mass and the fact that its distance has not been measured give it the status of a mysterious and enigmatic object. Located in the direction of the constellation.....\n#astronomy #space #astrophysics #astrophotography ",
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"content": "<a href=\"https://www.minds.com/search?f=top&t=all&q=UMPlus\" title=\"#UMPlus\" class=\"u-url hashtag\" target=\"_blank\">#UMPlus</a> - Propeller Nebula by David Lindemann<br /><br /><a href=\"https://www.universomagico.net/2025/06/nebulosa-propulsor-por-david-lindemann.html\" target=\"_blank\">https://www.universomagico.net/2025/06/nebulosa-propulsor-por-david-lindemann.html</a><br /><br />This spectacular image by astronomer David Lindemann primarily shows a striking cloud called the Propeller Nebula. It is also cataloged as Simeis 57 and has four designations in the DWB catalog based on its parts. The image displays a large amount of hydrogen, which is ionized by nearby hot, young stars. The Propeller Nebula is only a few tens of times the mass of the Sun. Its low mass and the fact that its distance has not been measured give it the status of a mysterious and enigmatic object. Located in the direction of the constellation.....<br /><a href=\"https://www.minds.com/search?f=top&t=all&q=astronomy\" title=\"#astronomy\" class=\"u-url hashtag\" target=\"_blank\">#astronomy</a> <a href=\"https://www.minds.com/search?f=top&t=all&q=space\" title=\"#space\" class=\"u-url hashtag\" target=\"_blank\">#space</a> <a href=\"https://www.minds.com/search?f=top&t=all&q=astrophysics\" title=\"#astrophysics\" class=\"u-url hashtag\" target=\"_blank\">#astrophysics</a> <a href=\"https://www.minds.com/search?f=top&t=all&q=astrophotography\" title=\"#astrophotography\" class=\"u-url hashtag\" target=\"_blank\">#astrophotography</a> ",
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"content": "#UMPlus - Propeller Nebula by David Lindemann\n\nhttps://www.universomagico.net/2025/06/nebulosa-propulsor-por-david-lindemann.html\n\nThis spectacular image by astronomer David Lindemann primarily shows a striking cloud called the Propeller Nebula. It is also cataloged as Simeis 57 and has four designations in the DWB catalog based on its parts. The image displays a large amount of hydrogen, which is ionized by nearby hot, young stars. The Propeller Nebula is only a few tens of times the mass of the Sun. Its low mass and the fact that its distance has not been measured give it the status of a mysterious and enigmatic object. Located in the direction of the constellation.....\n#astronomy #space #astrophysics #astrophotography ",
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"content": "<a href=\"https://www.minds.com/search?f=top&t=all&q=UMPlus\" title=\"#UMPlus\" class=\"u-url hashtag\" target=\"_blank\">#UMPlus</a> - Propeller Nebula by David Lindemann<br /><br /><a href=\"https://www.universomagico.net/2025/06/nebulosa-propulsor-por-david-lindemann.html\" target=\"_blank\">https://www.universomagico.net/2025/06/nebulosa-propulsor-por-david-lindemann.html</a><br /><br />This spectacular image by astronomer David Lindemann primarily shows a striking cloud called the Propeller Nebula. It is also cataloged as Simeis 57 and has four designations in the DWB catalog based on its parts. The image displays a large amount of hydrogen, which is ionized by nearby hot, young stars. The Propeller Nebula is only a few tens of times the mass of the Sun. Its low mass and the fact that its distance has not been measured give it the status of a mysterious and enigmatic object. Located in the direction of the constellation.....<br /><a href=\"https://www.minds.com/search?f=top&t=all&q=astronomy\" title=\"#astronomy\" class=\"u-url hashtag\" target=\"_blank\">#astronomy</a> <a href=\"https://www.minds.com/search?f=top&t=all&q=space\" title=\"#space\" class=\"u-url hashtag\" target=\"_blank\">#space</a> <a href=\"https://www.minds.com/search?f=top&t=all&q=astrophysics\" title=\"#astrophysics\" class=\"u-url hashtag\" target=\"_blank\">#astrophysics</a> <a href=\"https://www.minds.com/search?f=top&t=all&q=astrophotography\" title=\"#astrophotography\" class=\"u-url hashtag\" target=\"_blank\">#astrophotography</a> ",
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"published": "2025-06-12T19:46:17+00:00",
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"content": "#UMPlus - Propeller Nebula by David Lindemann\n\nhttps://www.universomagico.net/2025/06/nebulosa-propulsor-por-david-lindemann.html\n\nThis spectacular image by astronomer David Lindemann primarily shows a striking cloud called the Propeller Nebula. It is also cataloged as Simeis 57 and has four designations in the DWB catalog based on its parts. The image displays a large amount of hydrogen, which is ionized by nearby hot, young stars. The Propeller Nebula is only a few tens of times the mass of the Sun. Its low mass and the fact that its distance has not been measured give it the status of a mysterious and enigmatic object. Located in the direction of the constellation.....\n#astronomy #space #astrophysics #astrophotography ",
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"content": "<a href=\"https://www.minds.com/search?f=top&t=all&q=UMPlus\" title=\"#UMPlus\" class=\"u-url hashtag\" target=\"_blank\">#UMPlus</a> - Collinder 464<br /><br /><a href=\"https://www.universomagico.net/2025/06/collinder-464.html\" target=\"_blank\">https://www.universomagico.net/2025/06/collinder-464.html</a><br /><br />This bright group of stars theoretically forms the open star cluster Collinder 464, located toward the constellation Cameleopardalis. We say theoretically because many of the designations in the Collinder Catalogue are dubious in their classification as true clusters. In fact, many designations were already classified as asterisms, random alignments of stars, which together stand out from the rest from our perspective. There is no scientific literature on Collinder 464; if it is a star cluster, its member stars should share a proper motion. Its brightest star is.....<br /><a href=\"https://www.minds.com/search?f=top&t=all&q=astronomy\" title=\"#astronomy\" class=\"u-url hashtag\" target=\"_blank\">#astronomy</a> <a href=\"https://www.minds.com/search?f=top&t=all&q=space\" title=\"#space\" class=\"u-url hashtag\" target=\"_blank\">#space</a> <a href=\"https://www.minds.com/search?f=top&t=all&q=astrophysics\" title=\"#astrophysics\" class=\"u-url hashtag\" target=\"_blank\">#astrophysics</a> <a href=\"https://www.minds.com/search?f=top&t=all&q=astrophotography\" title=\"#astrophotography\" class=\"u-url hashtag\" target=\"_blank\">#astrophotography</a> ",
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"published": "2025-06-11T16:14:54+00:00",
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"content": "#UMPlus - Collinder 464\n\nhttps://www.universomagico.net/2025/06/collinder-464.html\n\nThis bright group of stars theoretically forms the open star cluster Collinder 464, located toward the constellation Cameleopardalis. We say theoretically because many of the designations in the Collinder Catalogue are dubious in their classification as true clusters. In fact, many designations were already classified as asterisms, random alignments of stars, which together stand out from the rest from our perspective. There is no scientific literature on Collinder 464; if it is a star cluster, its member stars should share a proper motion. Its brightest star is.....\n#astronomy #space #astrophysics #astrophotography ",
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"content": "<a href=\"https://www.minds.com/search?f=top&t=all&q=UMPlus\" title=\"#UMPlus\" class=\"u-url hashtag\" target=\"_blank\">#UMPlus</a> - Collinder 464<br /><br /><a href=\"https://www.universomagico.net/2025/06/collinder-464.html\" target=\"_blank\">https://www.universomagico.net/2025/06/collinder-464.html</a><br /><br />This bright group of stars theoretically forms the open star cluster Collinder 464, located toward the constellation Cameleopardalis. We say theoretically because many of the designations in the Collinder Catalogue are dubious in their classification as true clusters. In fact, many designations were already classified as asterisms, random alignments of stars, which together stand out from the rest from our perspective. There is no scientific literature on Collinder 464; if it is a star cluster, its member stars should share a proper motion. Its brightest star is.....<br /><a href=\"https://www.minds.com/search?f=top&t=all&q=astronomy\" title=\"#astronomy\" class=\"u-url hashtag\" target=\"_blank\">#astronomy</a> <a href=\"https://www.minds.com/search?f=top&t=all&q=space\" title=\"#space\" class=\"u-url hashtag\" target=\"_blank\">#space</a> <a href=\"https://www.minds.com/search?f=top&t=all&q=astrophysics\" title=\"#astrophysics\" class=\"u-url hashtag\" target=\"_blank\">#astrophysics</a> <a href=\"https://www.minds.com/search?f=top&t=all&q=astrophotography\" title=\"#astrophotography\" class=\"u-url hashtag\" target=\"_blank\">#astrophotography</a> ",
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"url": "https://www.minds.com/newsfeed/1779569719599177728",
"published": "2025-06-11T16:14:43+00:00",
"source": {
"content": "#UMPlus - Collinder 464\n\nhttps://www.universomagico.net/2025/06/collinder-464.html\n\nThis bright group of stars theoretically forms the open star cluster Collinder 464, located toward the constellation Cameleopardalis. We say theoretically because many of the designations in the Collinder Catalogue are dubious in their classification as true clusters. In fact, many designations were already classified as asterisms, random alignments of stars, which together stand out from the rest from our perspective. There is no scientific literature on Collinder 464; if it is a star cluster, its member stars should share a proper motion. Its brightest star is.....\n#astronomy #space #astrophysics #astrophotography ",
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"content": "<a href=\"https://www.minds.com/search?f=top&t=all&q=UMPlus\" title=\"#UMPlus\" class=\"u-url hashtag\" target=\"_blank\">#UMPlus</a> - Messier 104<br /><br /><a href=\"https://www.universomagico.net/2025/06/messier-104.html\" target=\"_blank\">https://www.universomagico.net/2025/06/messier-104.html</a><br /><br />Messier 104, or NGC 4594, is a lenticular galaxy located in the direction of the Virgo constellation and situated at a distance of about 30 million light-years from the Milky Way. Popularly known as the Sombrero Galaxy, it has a bright nucleus and an unusual central bulge. Viewed almost edge-on, it takes on the appearance of a Mexican hat, with a broad, flattened disk, dark dust lanes, and a pronounced glow. Messier 104 possesses a rich system of globular clusters, with an estimated population of over 2,000 of these stellar monsters, more than 100 of which are visible using large telescopes. Recent studies indicate that it has.....<br /><a href=\"https://www.minds.com/search?f=top&t=all&q=astronomy\" title=\"#astronomy\" class=\"u-url hashtag\" target=\"_blank\">#astronomy</a> <a href=\"https://www.minds.com/search?f=top&t=all&q=space\" title=\"#space\" class=\"u-url hashtag\" target=\"_blank\">#space</a> <a href=\"https://www.minds.com/search?f=top&t=all&q=astrophysics\" title=\"#astrophysics\" class=\"u-url hashtag\" target=\"_blank\">#astrophysics</a> <a href=\"https://www.minds.com/search?f=top&t=all&q=astrophotography\" title=\"#astrophotography\" class=\"u-url hashtag\" target=\"_blank\">#astrophotography</a> ",
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"url": "https://www.minds.com/newsfeed/1779250063353864192",
"published": "2025-06-10T19:04:31+00:00",
"source": {
"content": "#UMPlus - Messier 104\n\nhttps://www.universomagico.net/2025/06/messier-104.html\n\nMessier 104, or NGC 4594, is a lenticular galaxy located in the direction of the Virgo constellation and situated at a distance of about 30 million light-years from the Milky Way. Popularly known as the Sombrero Galaxy, it has a bright nucleus and an unusual central bulge. Viewed almost edge-on, it takes on the appearance of a Mexican hat, with a broad, flattened disk, dark dust lanes, and a pronounced glow. Messier 104 possesses a rich system of globular clusters, with an estimated population of over 2,000 of these stellar monsters, more than 100 of which are visible using large telescopes. Recent studies indicate that it has.....\n#astronomy #space #astrophysics #astrophotography ",
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"content": "<a href=\"https://www.minds.com/search?f=top&t=all&q=UMPlus\" title=\"#UMPlus\" class=\"u-url hashtag\" target=\"_blank\">#UMPlus</a> - Messier 104<br /><br /><a href=\"https://www.universomagico.net/2025/06/messier-104.html\" target=\"_blank\">https://www.universomagico.net/2025/06/messier-104.html</a><br /><br />Messier 104, or NGC 4594, is a lenticular galaxy located in the direction of the Virgo constellation and situated at a distance of about 30 million light-years from the Milky Way. Popularly known as the Sombrero Galaxy, it has a bright nucleus and an unusual central bulge. Viewed almost edge-on, it takes on the appearance of a Mexican hat, with a broad, flattened disk, dark dust lanes, and a pronounced glow. Messier 104 possesses a rich system of globular clusters, with an estimated population of over 2,000 of these stellar monsters, more than 100 of which are visible using large telescopes. Recent studies indicate that it has.....<br /><a href=\"https://www.minds.com/search?f=top&t=all&q=astronomy\" title=\"#astronomy\" class=\"u-url hashtag\" target=\"_blank\">#astronomy</a> <a href=\"https://www.minds.com/search?f=top&t=all&q=space\" title=\"#space\" class=\"u-url hashtag\" target=\"_blank\">#space</a> <a href=\"https://www.minds.com/search?f=top&t=all&q=astrophysics\" title=\"#astrophysics\" class=\"u-url hashtag\" target=\"_blank\">#astrophysics</a> <a href=\"https://www.minds.com/search?f=top&t=all&q=astrophotography\" title=\"#astrophotography\" class=\"u-url hashtag\" target=\"_blank\">#astrophotography</a> ",
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"published": "2025-06-10T19:04:18+00:00",
"source": {
"content": "#UMPlus - Messier 104\n\nhttps://www.universomagico.net/2025/06/messier-104.html\n\nMessier 104, or NGC 4594, is a lenticular galaxy located in the direction of the Virgo constellation and situated at a distance of about 30 million light-years from the Milky Way. Popularly known as the Sombrero Galaxy, it has a bright nucleus and an unusual central bulge. Viewed almost edge-on, it takes on the appearance of a Mexican hat, with a broad, flattened disk, dark dust lanes, and a pronounced glow. Messier 104 possesses a rich system of globular clusters, with an estimated population of over 2,000 of these stellar monsters, more than 100 of which are visible using large telescopes. Recent studies indicate that it has.....\n#astronomy #space #astrophysics #astrophotography ",
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"content": "<a href=\"https://www.minds.com/search?f=top&t=all&q=UMPlus\" title=\"#UMPlus\" class=\"u-url hashtag\" target=\"_blank\">#UMPlus</a> - NGC 3081 by Roberto Colombari<br /><br /><a href=\"https://www.universomagico.net/2025/06/ngc-3081-por-roberto-colombari.html\" target=\"_blank\">https://www.universomagico.net/2025/06/ngc-3081-por-roberto-colombari.html</a><br /><br /><a href=\"https://www.minds.com/groups/profile/1144295236524617728/feed\" target=\"_blank\">https://www.minds.com/groups/profile/1144295236524617728/feed</a><br /><br />This image by astronomer Roberto Colombari shows the galaxy NGC 3081, also known as IC 2529. It is located in the direction of the Hydra constellation and lies at a distance of about 85 million light-years from the Milky Way. Its classification is quite complex: it is a lenticular galaxy, a hybrid between a spiral and an elliptical. It is also a barred galaxy, as it has a bar composed of stars that runs through the galactic center. It is also a ring galaxy; ring galaxies are characterized by ring structures instead of the typical spiral arms. NGC 3081 is also a Seyfert 2 type, an energetic galaxy that hosts an active nucleus. This nucleus produces.....<br /><a href=\"https://www.minds.com/search?f=top&t=all&q=astronomy\" title=\"#astronomy\" class=\"u-url hashtag\" target=\"_blank\">#astronomy</a> <a href=\"https://www.minds.com/search?f=top&t=all&q=space\" title=\"#space\" class=\"u-url hashtag\" target=\"_blank\">#space</a> <a href=\"https://www.minds.com/search?f=top&t=all&q=astrophysics\" title=\"#astrophysics\" class=\"u-url hashtag\" target=\"_blank\">#astrophysics</a> <a href=\"https://www.minds.com/search?f=top&t=all&q=astrophotography\" title=\"#astrophotography\" class=\"u-url hashtag\" target=\"_blank\">#astrophotography</a> ",
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"content": "#UMPlus - NGC 3081 by Roberto Colombari\n\nhttps://www.universomagico.net/2025/06/ngc-3081-por-roberto-colombari.html\n\nhttps://www.minds.com/groups/profile/1144295236524617728/feed\n\nThis image by astronomer Roberto Colombari shows the galaxy NGC 3081, also known as IC 2529. It is located in the direction of the Hydra constellation and lies at a distance of about 85 million light-years from the Milky Way. Its classification is quite complex: it is a lenticular galaxy, a hybrid between a spiral and an elliptical. It is also a barred galaxy, as it has a bar composed of stars that runs through the galactic center. It is also a ring galaxy; ring galaxies are characterized by ring structures instead of the typical spiral arms. NGC 3081 is also a Seyfert 2 type, an energetic galaxy that hosts an active nucleus. This nucleus produces.....\n#astronomy #space #astrophysics #astrophotography ",
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"content": "<a href=\"https://www.minds.com/search?f=top&t=all&q=UMPlus\" title=\"#UMPlus\" class=\"u-url hashtag\" target=\"_blank\">#UMPlus</a> - NGC 3081 by Roberto Colombari<br /><br /><a href=\"https://www.universomagico.net/2025/06/ngc-3081-por-roberto-colombari.html\" target=\"_blank\">https://www.universomagico.net/2025/06/ngc-3081-por-roberto-colombari.html</a><br /><br />This image by astronomer Roberto Colombari shows the galaxy NGC 3081, also known as IC 2529. It is located in the direction of the Hydra constellation and lies at a distance of about 85 million light-years from the Milky Way. Its classification is quite complex: it is a lenticular galaxy, a hybrid between a spiral and an elliptical. It is also a barred galaxy, as it has a bar composed of stars that runs through the galactic center. It is also a ring galaxy; ring galaxies are characterized by ring structures instead of the typical spiral arms. NGC 3081 is also a Seyfert 2 type, an energetic galaxy that hosts an active nucleus. This nucleus produces.....<br /><a href=\"https://www.minds.com/search?f=top&t=all&q=astronomy\" title=\"#astronomy\" class=\"u-url hashtag\" target=\"_blank\">#astronomy</a> <a href=\"https://www.minds.com/search?f=top&t=all&q=space\" title=\"#space\" class=\"u-url hashtag\" target=\"_blank\">#space</a> <a href=\"https://www.minds.com/search?f=top&t=all&q=astrophysics\" title=\"#astrophysics\" class=\"u-url hashtag\" target=\"_blank\">#astrophysics</a> <a href=\"https://www.minds.com/search?f=top&t=all&q=astrophotography\" title=\"#astrophotography\" class=\"u-url hashtag\" target=\"_blank\">#astrophotography</a> ",
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"content": "#UMPlus - NGC 3081 by Roberto Colombari\n\nhttps://www.universomagico.net/2025/06/ngc-3081-por-roberto-colombari.html\n\nThis image by astronomer Roberto Colombari shows the galaxy NGC 3081, also known as IC 2529. It is located in the direction of the Hydra constellation and lies at a distance of about 85 million light-years from the Milky Way. Its classification is quite complex: it is a lenticular galaxy, a hybrid between a spiral and an elliptical. It is also a barred galaxy, as it has a bar composed of stars that runs through the galactic center. It is also a ring galaxy; ring galaxies are characterized by ring structures instead of the typical spiral arms. NGC 3081 is also a Seyfert 2 type, an energetic galaxy that hosts an active nucleus. This nucleus produces.....\n#astronomy #space #astrophysics #astrophotography ",
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"content": "<a href=\"https://www.minds.com/search?f=top&t=all&q=UMPlus\" title=\"#UMPlus\" class=\"u-url hashtag\" target=\"_blank\">#UMPlus</a> - NGC 3081 by Roberto Colombari<br /><br /><a href=\"https://www.universomagico.net/2025/06/ngc-3081-por-roberto-colombari.html\" target=\"_blank\">https://www.universomagico.net/2025/06/ngc-3081-por-roberto-colombari.html</a><br /><br />This image by astronomer Roberto Colombari shows the galaxy NGC 3081, also known as IC 2529. It is located in the direction of the Hydra constellation and lies at a distance of about 85 million light-years from the Milky Way. Its classification is quite complex: it is a lenticular galaxy, a hybrid between a spiral and an elliptical. It is also a barred galaxy, as it has a bar composed of stars that runs through the galactic center. It is also a ring galaxy; ring galaxies are characterized by ring structures instead of the typical spiral arms. NGC 3081 is also a Seyfert 2 type, an energetic galaxy that hosts an active nucleus. This nucleus produces.....<br /><a href=\"https://www.minds.com/search?f=top&t=all&q=astronomy\" title=\"#astronomy\" class=\"u-url hashtag\" target=\"_blank\">#astronomy</a> <a href=\"https://www.minds.com/search?f=top&t=all&q=space\" title=\"#space\" class=\"u-url hashtag\" target=\"_blank\">#space</a> <a href=\"https://www.minds.com/search?f=top&t=all&q=astrophysics\" title=\"#astrophysics\" class=\"u-url hashtag\" target=\"_blank\">#astrophysics</a> <a href=\"https://www.minds.com/search?f=top&t=all&q=astrophotography\" title=\"#astrophotography\" class=\"u-url hashtag\" target=\"_blank\">#astrophotography</a> ",
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"content": "#UMPlus - NGC 3081 by Roberto Colombari\n\nhttps://www.universomagico.net/2025/06/ngc-3081-por-roberto-colombari.html\n\nThis image by astronomer Roberto Colombari shows the galaxy NGC 3081, also known as IC 2529. It is located in the direction of the Hydra constellation and lies at a distance of about 85 million light-years from the Milky Way. Its classification is quite complex: it is a lenticular galaxy, a hybrid between a spiral and an elliptical. It is also a barred galaxy, as it has a bar composed of stars that runs through the galactic center. It is also a ring galaxy; ring galaxies are characterized by ring structures instead of the typical spiral arms. NGC 3081 is also a Seyfert 2 type, an energetic galaxy that hosts an active nucleus. This nucleus produces.....\n#astronomy #space #astrophysics #astrophotography ",
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"content": "<a href=\"https://www.minds.com/search?f=top&t=all&q=UMPlus\" title=\"#UMPlus\" class=\"u-url hashtag\" target=\"_blank\">#UMPlus</a> - Barnard 201<br /><br /><a href=\"https://www.universomagico.net/2025/06/barnard-201.html\" target=\"_blank\">https://www.universomagico.net/2025/06/barnard-201.html</a><br /><br />Barnard 201, visible in the center of this Digitized Sky Survey image, is a dark cloud located in the direction of the constellation Perseus, about 3 arc minutes west of NGC 869, the easternmost of the two clusters that make up the popular Perseus Double Cluster. Barnard 201 is a dense, dark cloud that stands out against the star-filled background. Stars are not missing in this region, but due to its density, the cloud obscures the stars behind it, creating the visual impression that there are no stars there. This raw image was extracted from DSS data, a survey that.....<br /><a href=\"https://www.minds.com/search?f=top&t=all&q=astronomy\" title=\"#astronomy\" class=\"u-url hashtag\" target=\"_blank\">#astronomy</a> <a href=\"https://www.minds.com/search?f=top&t=all&q=space\" title=\"#space\" class=\"u-url hashtag\" target=\"_blank\">#space</a> <a href=\"https://www.minds.com/search?f=top&t=all&q=astrophysics\" title=\"#astrophysics\" class=\"u-url hashtag\" target=\"_blank\">#astrophysics</a> <a href=\"https://www.minds.com/search?f=top&t=all&q=astrophotography\" title=\"#astrophotography\" class=\"u-url hashtag\" target=\"_blank\">#astrophotography</a> ",
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"content": "#UMPlus - Barnard 201\n\nhttps://www.universomagico.net/2025/06/barnard-201.html\n\nBarnard 201, visible in the center of this Digitized Sky Survey image, is a dark cloud located in the direction of the constellation Perseus, about 3 arc minutes west of NGC 869, the easternmost of the two clusters that make up the popular Perseus Double Cluster. Barnard 201 is a dense, dark cloud that stands out against the star-filled background. Stars are not missing in this region, but due to its density, the cloud obscures the stars behind it, creating the visual impression that there are no stars there. This raw image was extracted from DSS data, a survey that.....\n#astronomy #space #astrophysics #astrophotography ",
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"content": "<a href=\"https://www.minds.com/search?f=top&t=all&q=UMPlus\" title=\"#UMPlus\" class=\"u-url hashtag\" target=\"_blank\">#UMPlus</a> - Barnard 201<br /><br /><a href=\"https://www.universomagico.net/2025/06/barnard-201.html\" target=\"_blank\">https://www.universomagico.net/2025/06/barnard-201.html</a><br /><br />Barnard 201, visible in the center of this Digitized Sky Survey image, is a dark cloud located in the direction of the constellation Perseus, about 3 arc minutes west of NGC 869, the easternmost of the two clusters that make up the popular Perseus Double Cluster. Barnard 201 is a dense, dark cloud that stands out against the star-filled background. Stars are not missing in this region, but due to its density, the cloud obscures the stars behind it, creating the visual impression that there are no stars there. This raw image was extracted from DSS data, a survey that.....<br /><a href=\"https://www.minds.com/search?f=top&t=all&q=astronomy\" title=\"#astronomy\" class=\"u-url hashtag\" target=\"_blank\">#astronomy</a> <a href=\"https://www.minds.com/search?f=top&t=all&q=space\" title=\"#space\" class=\"u-url hashtag\" target=\"_blank\">#space</a> <a href=\"https://www.minds.com/search?f=top&t=all&q=astrophysics\" title=\"#astrophysics\" class=\"u-url hashtag\" target=\"_blank\">#astrophysics</a> <a href=\"https://www.minds.com/search?f=top&t=all&q=astrophotography\" title=\"#astrophotography\" class=\"u-url hashtag\" target=\"_blank\">#astrophotography</a> ",
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"content": "#UMPlus - Barnard 201\n\nhttps://www.universomagico.net/2025/06/barnard-201.html\n\nBarnard 201, visible in the center of this Digitized Sky Survey image, is a dark cloud located in the direction of the constellation Perseus, about 3 arc minutes west of NGC 869, the easternmost of the two clusters that make up the popular Perseus Double Cluster. Barnard 201 is a dense, dark cloud that stands out against the star-filled background. Stars are not missing in this region, but due to its density, the cloud obscures the stars behind it, creating the visual impression that there are no stars there. This raw image was extracted from DSS data, a survey that.....\n#astronomy #space #astrophysics #astrophotography ",
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"content": "<a href=\"https://www.minds.com/search?f=top&t=all&q=UMPlus\" title=\"#UMPlus\" class=\"u-url hashtag\" target=\"_blank\">#UMPlus</a> - Spiral Galaxy NGC 685<br /><br /><a href=\"https://www.universomagico.net/2025/06/galaxia-espiral-ngc-685.html\" target=\"_blank\">https://www.universomagico.net/2025/06/galaxia-espiral-ngc-685.html</a><br /><br />This bright galaxy filled with young stars was captured by the Hubble Space Telescope in this image. Called NGC 685, it lies about 64 million light-years from the Milky Way and is located in the direction of the constellation Eridanus. NGC 685 is classified as a barred spiral because its feathery spiral arms sprout from the ends of a bar of stars located at the center of the galaxy. The Milky Way is also a barred spiral, but our galaxy is almost twice the size of NGC 685. Astronomers used the.....<br /><a href=\"https://www.minds.com/search?f=top&t=all&q=astronomy\" title=\"#astronomy\" class=\"u-url hashtag\" target=\"_blank\">#astronomy</a> <a href=\"https://www.minds.com/search?f=top&t=all&q=space\" title=\"#space\" class=\"u-url hashtag\" target=\"_blank\">#space</a> <a href=\"https://www.minds.com/search?f=top&t=all&q=astrophysics\" title=\"#astrophysics\" class=\"u-url hashtag\" target=\"_blank\">#astrophysics</a> <a href=\"https://www.minds.com/search?f=top&t=all&q=astrophotography\" title=\"#astrophotography\" class=\"u-url hashtag\" target=\"_blank\">#astrophotography</a> ",
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"content": "#UMPlus - Spiral Galaxy NGC 685\n\nhttps://www.universomagico.net/2025/06/galaxia-espiral-ngc-685.html\n\nThis bright galaxy filled with young stars was captured by the Hubble Space Telescope in this image. Called NGC 685, it lies about 64 million light-years from the Milky Way and is located in the direction of the constellation Eridanus. NGC 685 is classified as a barred spiral because its feathery spiral arms sprout from the ends of a bar of stars located at the center of the galaxy. The Milky Way is also a barred spiral, but our galaxy is almost twice the size of NGC 685. Astronomers used the.....\n#astronomy #space #astrophysics #astrophotography ",
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