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#asteroidthreat β€” Public Fediverse posts

Live and recent posts from across the Fediverse tagged #asteroidthreat, aggregated by home.social.

  1. The #NEO population is roughly 100,000 at the size of about 60 m, and if we go all the way down to a few meters in size, the population of #NEAs β˜„οΈ is over a billion.

    #DART smashed into the 160 m, 5.5-million-ton #asteroid #Dimorphos. If you wanted to deflect an asteroid 10 times larger, you’d need 1,000 DARTs to get the same minuscule deflection.

    In April 2029, an #asteroid the size of an aircraft carrier 🚒 will be passing much closer than the Moon. astronomy.com/science/how-we-t

    #AsteroidThreat

  2. The #NEO population is roughly 100,000 at the size of about 60 m, and if we go all the way down to a few meters in size, the population of #NEAs β˜„οΈ is over a billion.

    #DART smashed into the 160 m, 5.5-million-ton #asteroid #Dimorphos. If you wanted to deflect an asteroid 10 times larger, you’d need 1,000 DARTs to get the same minuscule deflection.

    In April 2029, an #asteroid the size of an aircraft carrier 🚒 will be passing much closer than the Moon. astronomy.com/science/how-we-t

    #AsteroidThreat

  3. The #NEO population is roughly 100,000 at the size of about 60 m, and if we go all the way down to a few meters in size, the population of #NEAs β˜„οΈ is over a billion.

    #DART smashed into the 160 m, 5.5-million-ton #asteroid #Dimorphos. If you wanted to deflect an asteroid 10 times larger, you’d need 1,000 DARTs to get the same minuscule deflection.

    In April 2029, an #asteroid the size of an aircraft carrier 🚒 will be passing much closer than the Moon. astronomy.com/science/how-we-t

    #AsteroidThreat

  4. The #NEO population is roughly 100,000 at the size of about 60 m, and if we go all the way down to a few meters in size, the population of #NEAs β˜„οΈ is over a billion.

    #DART smashed into the 160 m, 5.5-million-ton #asteroid #Dimorphos. If you wanted to deflect an asteroid 10 times larger, you’d need 1,000 DARTs to get the same minuscule deflection.

    In April 2029, an #asteroid the size of an aircraft carrier 🚒 will be passing much closer than the Moon. astronomy.com/science/how-we-t

    #AsteroidThreat

  5. The #NEO population is roughly 100,000 at the size of about 60 m, and if we go all the way down to a few meters in size, the population of #NEAs β˜„οΈ is over a billion.

    #DART smashed into the 160 m, 5.5-million-ton #asteroid #Dimorphos. If you wanted to deflect an asteroid 10 times larger, you’d need 1,000 DARTs to get the same minuscule deflection.

    In April 2029, an #asteroid the size of an aircraft carrier 🚒 will be passing much closer than the Moon. astronomy.com/science/how-we-t

    #AsteroidThreat

  6. Objects larger than 140 meters πŸ“ are closely tracked as they could cause significant regional damage if they impact πŸ’₯, yet scientists estimate that only about 40% πŸ“Š of these mid-sized #NEOs have been identified so far. Among the newly identified objects are 33 previously unknown #NEOs, the largest is about 500 meters wide. #Rubin is expected to reveal an additional 90,000 new NEOs, some of which may be potentially hazardous rubinobservatory.org/news/1100

    #RubinObservatory #AsteroidThreat

  7. Objects larger than 140 meters πŸ“ are closely tracked as they could cause significant regional damage if they impact πŸ’₯, yet scientists estimate that only about 40% πŸ“Š of these mid-sized #NEOs have been identified so far. Among the newly identified objects are 33 previously unknown #NEOs, the largest is about 500 meters wide. #Rubin is expected to reveal an additional 90,000 new NEOs, some of which may be potentially hazardous rubinobservatory.org/news/1100

    #RubinObservatory #AsteroidThreat

  8. Objects larger than 140 meters πŸ“ are closely tracked as they could cause significant regional damage if they impact πŸ’₯, yet scientists estimate that only about 40% πŸ“Š of these mid-sized #NEOs have been identified so far. Among the newly identified objects are 33 previously unknown #NEOs, the largest is about 500 meters wide. #Rubin is expected to reveal an additional 90,000 new NEOs, some of which may be potentially hazardous rubinobservatory.org/news/1100

    #RubinObservatory #AsteroidThreat

  9. Objects larger than 140 meters πŸ“ are closely tracked as they could cause significant regional damage if they impact πŸ’₯, yet scientists estimate that only about 40% πŸ“Š of these mid-sized #NEOs have been identified so far. Among the newly identified objects are 33 previously unknown #NEOs, the largest is about 500 meters wide. #Rubin is expected to reveal an additional 90,000 new NEOs, some of which may be potentially hazardous rubinobservatory.org/news/1100

    #RubinObservatory #AsteroidThreat

  10. Objects larger than 140 meters πŸ“ are closely tracked as they could cause significant regional damage if they impact πŸ’₯, yet scientists estimate that only about 40% πŸ“Š of these mid-sized #NEOs have been identified so far. Among the newly identified objects are 33 previously unknown #NEOs, the largest is about 500 meters wide. #Rubin is expected to reveal an additional 90,000 new NEOs, some of which may be potentially hazardous rubinobservatory.org/news/1100

    #RubinObservatory #AsteroidThreat

  11. The most unsettling thing about the #Chelyabinsk β˜„οΈ event is that nobody saw it coming. The explosion πŸ’₯ created a shockwave that is estimated to have released around 30 times more energy than the atomic bomb detonated at Hiroshima, damaging 7,200 buildings across six cities and sending 1,500 people to local hospitals and clinics with injuries. If the #asteroid had hit the ground intact, the damage could have been unlike anything in human history planetary.org/articles/what-wa

    #AsteroidThreat

  12. The most unsettling thing about the #Chelyabinsk β˜„οΈ event is that nobody saw it coming. The explosion πŸ’₯ created a shockwave that is estimated to have released around 30 times more energy than the atomic bomb detonated at Hiroshima, damaging 7,200 buildings across six cities and sending 1,500 people to local hospitals and clinics with injuries. If the #asteroid had hit the ground intact, the damage could have been unlike anything in human history planetary.org/articles/what-wa

    #AsteroidThreat

  13. The #meteor β˜„οΈ, measuring about 1 meter wide πŸ“, entered the atmosphere traveling at 120,000 kilometers per hour when it broke apart at an altitude of 64 kilometers. It released energy equivalent to about 300 tons of TNT πŸ’₯ dw.com/en/meteor-explodes-over

    πŸ“Š 453 fireball sightings in 2026 fireball.amsmeteors.org//membe

    #AsteroidThreat

  14. The #meteor β˜„οΈ, measuring about 1 meter wide πŸ“, entered the atmosphere traveling at 120,000 kilometers per hour when it broke apart at an altitude of 64 kilometers. It released energy equivalent to about 300 tons of TNT πŸ’₯ dw.com/en/meteor-explodes-over

    πŸ“Š 453 fireball sightings in 2026 fireball.amsmeteors.org//membe

    #AsteroidThreat

  15. β€œYou can only do something to address a threat if you know about it,” Moissl says. β€œSo the very first step in the whole chain is observations πŸ”­. You need to find the #asteroids.” sciencefocus.com/space/asteroi

    "If necessary, we can build a spacecraft to deflect an #asteroid β˜„οΈ in four years" ⏳πŸ₯± mundoamerica.com/entertainment

    #ESA #AsteroidThreat

  16. β€œYou can only do something to address a threat if you know about it,” Moissl says. β€œSo the very first step in the whole chain is observations πŸ”­. You need to find the #asteroids.” sciencefocus.com/space/asteroi

    "If necessary, we can build a spacecraft to deflect an #asteroid β˜„οΈ in four years" ⏳πŸ₯± mundoamerica.com/entertainment

    #ESA #AsteroidThreat

  17. #Asteroid #2017SH33 β˜„οΈ was last observed πŸ”­ in 2017 ssd.jpl.nasa.gov/tools/sbdb_lo and estimated 700m-1.6 km in diameter neo.ssa.esa.int/risk-list. It might impact πŸ’₯ 2026-04-30 (but we haven't a clue as there isn't any recent data)

    #NASA #ESA #AsteroidThreat #Astronomy

  18. #Asteroid #2017SH33 β˜„οΈ was last observed πŸ”­ in 2017 ssd.jpl.nasa.gov/tools/sbdb_lo and estimated 700m-1.6 km in diameter neo.ssa.esa.int/risk-list. It might impact πŸ’₯ 2026-04-30 (but we haven't a clue as there isn't any recent data)

    #NASA #ESA #AsteroidThreat #Astronomy

  19. The #meteorite β˜„οΈ crashed through the roof of a two-story house. It hit the floor in a bedroom, where it ricocheted and struck another part of the ceiling nytimes.com/2026/03/22/us/mete

    #AsteroidThreat #Houston

  20. The #meteorite β˜„οΈ crashed through the roof of a two-story house. It hit the floor in a bedroom, where it ricocheted and struck another part of the ceiling nytimes.com/2026/03/22/us/mete

    #AsteroidThreat #Houston

  21. #NASA’s #NEOSurveyor mission is now slated for no earlier than πŸ“† mid-2027, will spend at least five years scanning for potentially hazardous #asteroids β˜„οΈ larger than 140 meters.

    #NEOHunter - nearly nine times more massive than #DART - could execute a direct high-energy impact πŸ’₯, delivering approximately 1.5 times the kinetic energy
    nasaspaceflight.com/2026/03/bl

    #BlueOrigin #AsteroidThreat

  22. #NASA’s #NEOSurveyor mission is now slated for no earlier than πŸ“† mid-2027, will spend at least five years scanning for potentially hazardous #asteroids β˜„οΈ larger than 140 meters.

    #NEOHunter - nearly nine times more massive than #DART - could execute a direct high-energy impact πŸ’₯, delivering approximately 1.5 times the kinetic energy
    nasaspaceflight.com/2026/03/bl

    #BlueOrigin #AsteroidThreat

  23. #LSST performs very well for large impactors β˜„οΈ, discovering about 79.7% of objects larger than 140 m before impact. Only 50.3% of 50–140 m impactors, 26.8% of 20–50 m impactors, and 10.5% of 10–20 m impactors are discovered πŸ”­ at all. About 60% of large impactors fail to reach a one-year warning threshold. Upper mid-size objects are usually discovered only a few months before impact πŸ’₯ newplanetarium.com/journal/202

    #RubinObservatory #AsteroidThreat

  24. #LSST performs very well for large impactors β˜„οΈ, discovering about 79.7% of objects larger than 140 m before impact. Only 50.3% of 50–140 m impactors, 26.8% of 20–50 m impactors, and 10.5% of 10–20 m impactors are discovered πŸ”­ at all. About 60% of large impactors fail to reach a one-year warning threshold. Upper mid-size objects are usually discovered only a few months before impact πŸ’₯ newplanetarium.com/journal/202

    #RubinObservatory #AsteroidThreat

  25. A solution to mitigate low #deflection efficiency is to apply multiple low-energy impactors rather than a single high-energy impactor πŸ’₯. A lower kinetic energy impactor results in a smaller crater πŸ•³οΈ that is less affected by global curvature, increasing momentum transfer efficiency nature.com/articles/s41467-025

    #DART #AsteroidDeflection #AsteroidThreat

  26. A solution to mitigate low #deflection efficiency is to apply multiple low-energy impactors rather than a single high-energy impactor πŸ’₯. A lower kinetic energy impactor results in a smaller crater πŸ•³οΈ that is less affected by global curvature, increasing momentum transfer efficiency nature.com/articles/s41467-025

    #DART #AsteroidDeflection #AsteroidThreat

  27. A solution to mitigate low #deflection efficiency is to apply multiple low-energy impactors rather than a single high-energy impactor πŸ’₯. A lower kinetic energy impactor results in a smaller crater πŸ•³οΈ that is less affected by global curvature, increasing momentum transfer efficiency nature.com/articles/s41467-025

    #DART #AsteroidDeflection #AsteroidThreat

  28. A solution to mitigate low #deflection efficiency is to apply multiple low-energy impactors rather than a single high-energy impactor πŸ’₯. A lower kinetic energy impactor results in a smaller crater πŸ•³οΈ that is less affected by global curvature, increasing momentum transfer efficiency nature.com/articles/s41467-025

    #DART #AsteroidDeflection #AsteroidThreat

  29. A solution to mitigate low #deflection efficiency is to apply multiple low-energy impactors rather than a single high-energy impactor πŸ’₯. A lower kinetic energy impactor results in a smaller crater πŸ•³οΈ that is less affected by global curvature, increasing momentum transfer efficiency nature.com/articles/s41467-025

    #DART #AsteroidDeflection #AsteroidThreat

  30. Any useful deflection of a larger #asteroid β˜„οΈ would require a far greater shove or need to occur decades ahead of an impending collision πŸ’₯ to have a cumulative effect. You’d need 1,000 #DARTs to get the same deflection astronomy.com/science/how-we-t

    Discovery πŸ”­
    after closest approach: 69 (46.0%)
    < 24 hours : 32 (21.3%)
    up to 7 days : 47 (31.3%)
    > one week : 2 (1.3%)
    > 7 weeks : 0 (0.0%)
    > one year : 0 (0.0%)
    en.wikipedia.org/wiki/List_of_

    #Dimorphos #Didymos #AsteroidThreat #AsteroidDeflection #NASA #DART

  31. Any useful deflection of a larger #asteroid β˜„οΈ would require a far greater shove or need to occur decades ahead of an impending collision πŸ’₯ to have a cumulative effect. You’d need 1,000 #DARTs to get the same deflection astronomy.com/science/how-we-t

    Discovery πŸ”­
    after closest approach: 69 (46.0%)
    < 24 hours : 32 (21.3%)
    up to 7 days : 47 (31.3%)
    > one week : 2 (1.3%)
    > 7 weeks : 0 (0.0%)
    > one year : 0 (0.0%)
    en.wikipedia.org/wiki/List_of_

    #Dimorphos #Didymos #AsteroidThreat #AsteroidDeflection #NASA #DART

  32. Any useful deflection of a larger #asteroid β˜„οΈ would require a far greater shove or need to occur decades ahead of an impending collision πŸ’₯ to have a cumulative effect. You’d need 1,000 #DARTs to get the same deflection astronomy.com/science/how-we-t

    Discovery πŸ”­
    after closest approach: 69 (46.0%)
    < 24 hours : 32 (21.3%)
    up to 7 days : 47 (31.3%)
    > one week : 2 (1.3%)
    > 7 weeks : 0 (0.0%)
    > one year : 0 (0.0%)
    en.wikipedia.org/wiki/List_of_

    #Dimorphos #Didymos #AsteroidThreat #AsteroidDeflection #NASA #DART

  33. Any useful deflection of a larger #asteroid β˜„οΈ would require a far greater shove or need to occur decades ahead of an impending collision πŸ’₯ to have a cumulative effect. You’d need 1,000 #DARTs to get the same deflection astronomy.com/science/how-we-t

    Discovery πŸ”­
    after closest approach: 69 (46.0%)
    < 24 hours : 32 (21.3%)
    up to 7 days : 47 (31.3%)
    > one week : 2 (1.3%)
    > 7 weeks : 0 (0.0%)
    > one year : 0 (0.0%)
    en.wikipedia.org/wiki/List_of_

    #Dimorphos #Didymos #AsteroidThreat #AsteroidDeflection #NASA #DART

  34. Any useful deflection of a larger #asteroid β˜„οΈ would require a far greater shove or need to occur decades ahead of an impending collision πŸ’₯ to have a cumulative effect. You’d need 1,000 #DARTs to get the same deflection astronomy.com/science/how-we-t

    Discovery πŸ”­
    after closest approach: 69 (46.0%)
    < 24 hours : 32 (21.3%)
    up to 7 days : 47 (31.3%)
    > one week : 2 (1.3%)
    > 7 weeks : 0 (0.0%)
    > one year : 0 (0.0%)
    en.wikipedia.org/wiki/List_of_

    #Dimorphos #Didymos #AsteroidThreat #AsteroidDeflection #NASA #DART

  35. #2025SC79 is the second-fastest #asteroid β˜„οΈ, roughly 700 meters long, spotted on Sept. 27 hiding in the sun's β˜€οΈ glare. "The most #dangerous asteroids are the most difficult to detect" πŸ”­ space.com/astronomy/asteroids/

    #AsteroidThreat

  36. #2025SC79 is the second-fastest #asteroid β˜„οΈ, roughly 700 meters long, spotted on Sept. 27 hiding in the sun's β˜€οΈ glare. "The most #dangerous asteroids are the most difficult to detect" πŸ”­ space.com/astronomy/asteroids/

    #AsteroidThreat

  37. #Roman has the high sensitivity to measure the physical properties, compositions, and orbital trajectories of #NEOs β˜„οΈ in order to understand their physical nature and potential #hazards to Earth. Roman's #PlanetaryDefense capabilities complement those of the operational ground-based @VRubinObs πŸ”­ and the upcoming #space-based 🌌 #NEOSurveyor arxiv.org/abs/2508.14412

    πŸš€ October 2026 - May 2027 nextspaceflight.com/launches/d

    #AsteroidThreat #SpaceTelescope #RomanSpaceTelescope

  38. #Roman has the high sensitivity to measure the physical properties, compositions, and orbital trajectories of #NEOs β˜„οΈ in order to understand their physical nature and potential #hazards to Earth. Roman's #PlanetaryDefense capabilities complement those of the operational ground-based @VRubinObs πŸ”­ and the upcoming #space-based 🌌 #NEOSurveyor arxiv.org/abs/2508.14412

    πŸš€ October 2026 - May 2027 nextspaceflight.com/launches/d

    #AsteroidThreat #SpaceTelescope #RomanSpaceTelescope