Near earth objects 2023
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Home / near Earth objects. Tag: near Earth objects. Posted in Civil China to launch near-Earth asteroid sample return mission in 2025. 2025 Septem. Posted in Civil
Near-Earth Objects – Near-Earth Object Surveyor - NASA Blogs
NASA's top expert on near-Earth objects says that new telescope systems, including a "last alert" system that's just now being set up, are gradually getting a handle on potentially threatening asteroids. But comets? That's a completely different story."We can do something about asteroids. Comets are a problem," said Donald Yeomans, the head of the Near-Earth Object Program at NASA's Jet Propulsion Laboratory in Pasadena, Calif.Yeomans is the author of "Near-Earth Objects: Finding Them Before They Find Us," a new book sizing up the cosmic perils posed by asteroids and comets — and looking ahead to the potential they offer for scientific discovery and economic exploitation.For an example of the perils, you need look no further than the dinosaurs — or, more accurately, the lack thereof. Scientists believe an asteroid impact along the coast of Mexico's Yucatan Peninsula set off a chain of events that killed off the dinosaurs and many other species 65 million years ago. A much smaller impact in 1908 blew down half a million acres' worth of trees in Siberia, and could have leveled a city nearly the size of Tokyo if its trajectory were different.Donald Yeomans is manager of Near Earth Object Program Office.NASA / JPL-Caltech"Near-Earth Objects" focuses on the peril and the potential of asteroids and comets.Princeton U. PressMore recently, astronomers have sounded a series of alerts over close encounters with passing asteroids — including three cases involving the asteroids 2012 DA14, 2011 AG5 and Apophis. It turns out that none of those space rocks will hit us in the foreseeable future, but 2012 DA14 is due to come within 13,000 miles on Feb. 15. That's closer than the orbits for geosynchronous satellites. And experts agree it's only a matter of time before astronomers find a large asteroid that's actually on a collision course.This is why Congress asked NASA in 1998 to identify 90 percent of the asteroids wider than a kilometer (0.6 miles). In 2011, NASA researchers declared that they achieved that goal. But they still have a long way to go to identify the smaller threats: The experts estimate that there are more than a million near-Earth asteroids capable of causing damage on the scale of 1908's Siberian fireball.Several projects are in the works to catalog those smaller asteroid threats, including some projects that are funded by NASA's observation program for near-Earth objects, which is allocated more than $20 million annually. One such program — known as the Asteroid Terrestrial-impact Last Alert System, or ATLAS — started receiving NASA funding just this month. The $5 million, five-year effort calls for building telescopes in Hawaii that could provide advance warning for the kinds of asteroids that have eluded bigger detection programs."We think it's possible Georgina RannardClimate and science reporterGetty ImagesA large asteroid known as 2024 YR4 has grabbed headlines this week as scientists first raised its chances of hitting earth, then lowered them.The latest estimate says the object has a 0.28% chance of hitting Earth in 2032, significantly lower than the 3.1% chance earlier in the week.Scientists say it is now more likely to smash into the Moon, with Nasa estimating the probability of that happening at 1%.But in the time since 2024 YR4 was first spotted through a telescope in the desert in Chile two months ago, tens of other objects have passed closer to Earth than the Moon, which in astronomical terms sounds like a near miss.It is likely that others, albeit much smaller, have hit us or burned up in the atmosphere but gone unnoticed.This is the story of the asteroids that you never hear about – the fly-bys, the near-misses and the direct hits. The vast majority are harmless. But some carry the most valuable clues for unlocking mysteries in our universe, information we are desperate to get our hands on.Drs. Bill and Eileen Ryan, Magdalena Ridge Observatory 2.4m Telescope, New Mexico Tech2024 YR4 was first detected in December and there is small chance it could hit Earth on 22 December 2032Asteroids, also sometimes called minor planets, are rocky pieces left over from the formation of our solar system about 4.6 billion years ago.Rocks routinely orbit close to Earth, pushed by the gravity of other planets. For most of human history, it has been impossible to know how close we have come to being struck by a large asteroid. Serious monitoring of objects near Earth only started in the late 20th century, explains Professor Mark Boslough from the University of New Mexico. "Before that we were blissfully oblivious to them," he says.We now know that quite large objects - 40m across or more - pass between Earth and the Moon several times a year. That's the same size of asteroid that exploded over Siberia in 1908 injuring people and damaging buildings over 200 square miles.The most serious near-miss, and the closest comparison with YR4, was an asteroid called Apophis which was first spotted in 2004 and measured 375 meters across, or around the size of a cruise ship.Professor Patrick Michel from French National Centre for Scientific Research (CNRS) tracked Apophis and recalls it was considered the most hazardous asteroid ever detected.It took until 2013 to get enough observations to understand that it was not going to hit Earth.But he says there was one big difference with YR4. "We didn't know what to do. We discovered something, we determined an impact probability, and then thought, who do we call?" he says. Scientists and governments had no idea how to respond, he says.A large asteroid strike could be catastrophic if it hits an area where humans live. We don't know exactly how big YR4 is yet, but if it is at the top end of estimates, about 90m across, it would likelyNear Earth Objects - an overview
Or different from an electrical interaction? Explain. Tutorials in JntroducJOry Physics McDennott, Shaffer, & P.E.G., U. Wash. ©Prentice Hall, Inc. First Edition, 2002 Magnets and magnetic fields EM 115 II. Magnetic fields We have observed that magnets interact even when they are not in direct contact. In electrostatics we used the idea of an electric field to account for the interaction between charges that were separated from one another. For magnetic interactions, we similarly define a magnetic field. A. Obtain a compass from a tutorial instructor. 1. Use the compass to explore the region around a bar magnet. Describe the behavior of the compass needle both near the poles of the magnet and in the region between the poles. To which class of objects from section I does the compass needle belong? Explain. 2. Move the compass far away from all other objects. Shake the compass and describe the behavior of the compass needle. Does the needle behave as if it is in a magnetic field? We can account for the behavior of the compass needle by supposing that it interacts with the Earth and that the Earth belongs to one of the categories from section I. To which class of objects from section I do your observations suggest the Earth belongs? Explain how you can tell. 3. We define the north pole of a magnet as the end that points toward the arctic region of the Earth when the magnet is free to rotate and is not interacting with. Home / near Earth objects. Tag: near Earth objects. Posted in Civil China to launch near-Earth asteroid sample return mission in 2025. 2025 Septem. Posted in Civil Collection . Planetary Defense, Space Debris and Near-Earth Objects. With the increasing presence of space debris and the potential risk posed by near-Earth objects (NEOsNear-Earth Object Program - NASA
Massive 800-foot asteroid closely past the Earth. (Credit- Freepik)A huge stadium-sized space rock, the Asteroid 2023 SP1 cruised towards the Earth at a close distance today, NASA has confirmed. Asteroids, the rocky remnants of our solar system's formation, have left a deep mark on Earth in the form of craters, some colossal, some barely appearing on the landscape. These craters tell stories of scary collisions. Smaller asteroids, mere pebbles in the cosmic game, create fleeting streaks of light as meteors before burning up in our atmosphere. These leave behind no permanent mark, except for the occasional meteorite, a piece that survives the fiery destruction. Thankfully, the massive 800-foot asteroid escaped the Earth. Here is what NASA has revealed.Asteroid 2023 SP1: Key CharacteristicsAccording to NASA CNEOs data, this 800-foot extremely massive stadium-sized near-Earth object travelled towards Earth at a furious speed of 42480 kilometres per hour. The space rock made its closest approach to Earth today, February 7, 2024, passing at a close distance of a mere 3.41 million miles. And yes, the Asteroid 2008 OS7 was classified as a Potentially Hazardous Asteroid (PHA) by NASA's Center for Near-Earth Object Studies (CNEOS) due to its huge size and close approach towards the Earth.Asteroids and their potential to impact EarthMassive asteroids have played a significant role in shaping the history of Earth, both in terms of geological processes and the evolution of life. These celestial bodies, often remnants from the early solar system, are composed of rock, metal, and other materials. While most asteroids are relatively small and orbit the Sun within the asteroid belt between Mars and Jupiter, there is a potential threat posed by larger asteroids that could collide with Earth. Their impact on Earth has the potential to cause catastrophic consequences.The potential risk of a massive asteroid impact remains a concern, and ongoing research and preparedness are crucial to understanding and mitigating this potential threat. Advances in technology and international collaboration will continue to play a vital role in monitoring and responding to the ever-present cosmic hazards that our planet faces. Sisto, A. Brunini, L.D. Dirani, R.B. Orellana, Hilda asteroids among Jupiter family comets. Icarus 174(1), 81–89 (2005)Article ADS Google Scholar P. Farinella, C. Froeschlé, C. Froeschlé, R. Gonczi, G. Hahn, A. Morbidelli, G.B. Valsecchi, Asteroids falling into the sun. Nature 371(6495), 314–317 (1994)Article ADS Google Scholar J.A. Fernández, T. Gallardo, A. Brunini, Are there many inactive Jupiter-family comets among the near-earth asteroid population? Icarus 159(2), 358–368 (2002)Article ADS Google Scholar J.A. Fernández, T. Gallardo, A. Brunini, Are there many inactive Jupiter-family comets among the near-earth asteroid population? Icarus 159(2), 358–368 (2002). ADS Google Scholar J.A. Fernández, A. Sosa, T. Gallardo, J.N. Gutiérrez, Assessing the physical nature of near-earth asteroids through their dynamical histories. Icarus 238, 1–12 (2014). ADS Google Scholar T. Gallardo, Atlas of the mean motion resonances in the solar system. Icarus 184(1), 29–38 (2006). ADS Google Scholar B.J. Gladman, F. Migliorini, A. Morbidelli, V. Zappala, P. Michel, A. Cellino, C. Froeschle, H.F. Levison, M. Bailey, M. Duncan, Dynamical lifetimes of objects injected into asteroid belt resonances. Science 277(5323), 197–201 (1997)Article ADS Google Scholar B. Gladman, P. Michel, C. Froeschlé, The near-earth object population. Icarus 146(1), 176–189 (2000)Article ADS Google Scholar M. Granvik, A. Morbidelli, R. Jedicke, B. Bolin, W.F. Bottke, E. Beshore, D. Vokrouhlickỳ, M. Delbò, P. Michel, Super-catastrophic disruption of asteroids at small perihelion distances. Nature 530(7590), 303–306 (2016)Article ADS Google Scholar M. Granvik, A. Morbidelli, D. Vokrouhlickỳ, W.F. Bottke, D. Nesvornỳ, R. Jedicke, Escape of asteroids from the main belt. Astron. Astrophys. 598, A52 (2017)Article ADSNear-Earth Objects Discovered to Date
Jorba, À., Jorba-Cuscó, M.: Invariant manifolds near \({L}_1\) and \({L}_2\) in the quasi-bicircular problem. Celestial Mech. Dyn. Astron. 135(15). (2023)Sanaga, R.R., Howell, K.: Analyzing the Challenging Region in the Earth-Moon L\(_2\) Halo Family via Hill Restricted Four-Body Problem Dynamics. In: AIAA SCITECH 2024 Forum, (2024)Sanaga, R.R., Howell, K.C.: Synodic resonant halo orbits in the Hill restricted four-body problem. In: 33rd AAS/AIAA Spaceflight Mechanics Meeting, Austin, Texas, January 15-19, 2023 (2023)Scheeres, D.J.: The Restricted Hill Four-Body Problem with Applications to the Earth-Moon-Sun system. Celest. Mech. Dyn. Astron. 70, 75–98 (1998). ADS MathSciNet MATH Google Scholar Szebehely, V.: Theory of Orbit: The Restricted Problem of Three Bodies. Academic Press (1967). D., Baresi, N., Locoche, S., et al.: Resonant quasi-periodic near-rectilinear Halo orbits in the Elliptic-Circular Earth-Moon-Sun Problem. Adv. Space Res. 71(1), 336–354 (2023). ADS Google Scholar Wintner, A.: The Analytical Foundations of Celestial Mechanics. Princeton University Press (1947)MATH Google Scholar Zimovan-Spreen, E.M., Howell, K.C., Davis, D.C.: Near rectilinear halo orbits and nearby higher-period dynamical structures: orbital stability and resonance properties. Celest. Mech. Dyn. Astron. 132(5), 28 (2020). ADS MathSciNet MATH Google Scholar Zimovan-Spreen, E.M., Scheuerle, S.T., McCarthy, B.P., et al. Baseline Orbit Generation for Near Rectilinear Halo Orbits. In: AAS/AAIA Astrodynamics Specialist Conference, Big Sky, Montana, August 13-17, 2023 (2023)Download referencesAcknowledgementsValuable discussions with members from Multi-Body Dynamics Research Group are appreciated. Beom Park would like to thank Kwanjeong Educational Foundation for the financial support. Rohith Reddy Sanaga would like to thank Department of Computer Science Department at Purdue University. Portions of this work are also supported by Purdue University and under Grant NASA JSC 80NSSC18M0122.Author informationAuthors and AffiliationsSchool of Aeronautics and Astronautics, Purdue University, 610 Purdue Mall, West Lafayette, IN, 47907, USABeom Park, Rohith Reddy Sanaga & Kathleen C. HowellAuthorsBeom ParkYou can also search for this author in PubMed Google ScholarRohith Reddy SanagaYou can also search for this author in PubMed Google ScholarKathleen C. HowellYou can also search for this author in PubMed Google ScholarCorresponding authorCorrespondence to Beom Park.Additional informationPublisher's NoteSpringer Nature remains neutral with regard to jurisdictional claims in published maps and institutional affiliations.AppendicesAppendix A Review of the QBCP expressions from Andreu (1998)The expressions that appear in the original derivation of the QBCP from Andreu (1998) are reviewed. A group of coefficients, \(\alpha _{k}\), \(1 \le k \le 8\), appear with the following physical interpretations, (A1) The \(\alpha _{k}\) functions are assumed in the following forms,$$\begin{aligned} \alpha _{k} = \sum _j \alpha _{kj} \cos (j t_*), & k = 1, 3, 4, 6, 7 \nonumber \\ \alpha _{k} = \sum _j \alpha _{kj} \sin (j t_*), & k = 2, 5, 8, \end{aligned}$$ (A2) where sines and cosines coefficients \(\alpha _{kj}\) are included in Tables 3, 4, and 5. Note that(PDF) Near-Earth Objects - ResearchGate
The Solar system are. It is located between Mars and Jupiter and it is believed to have formed because Jupiter is so big that its gravity stopped other planets from forming nearby, resulting in the fragmentation of the material into asteroids.There are over 1 million large asteroids in the asteroid belt (larger than 1 kilometer or 0.6 miles) and there are millions more that are smaller than that.Ceres, one of the asteroids in the belt is so big that it is considered both an asteroid and a dwarf planet. Check out our article about the 8 most famous and important asteroids for more on that.Trojan asteroidsTrojan asteroids are very interesting. They get their name from a group of asteroids discovered in Jupiter’s orbit.These asteroids share an orbit with a planet, but they don’t collide with it because they are located at very exact points of their orbits in the “Lagrange points” (approximately at 60° of the planet), forming a balance.Jupiter is the planet with the most trojans in its orbit, so many have been discovered in recent years that it is now believed there could be as many as in the asteroid belt.The rest of the planets only have a few trojans with the second place being taken by Neptune with 30. Earth has two called 2010 TK7, and 2020 XL5.Near-Earth asteroidsThese are asteroids that have an orbit outside the major groups. Their trajectory passes near Earth’s orbit and in some cases, it even crosses it.Near-Earth asteroids are also commonly called NEOs (Near-Earth Objects) and there are currently 30,503 detected ones that are being constantly monitored as these are the one that represents the most danger to Earth. Most of them are asteroids, but a few NEOs can also be comets.For an object to be considered a NEO, the closest point of its orbit (perihelion) to the Sun has to be less than 1.3 Astronomical Units (1 AU = the average distance between the Sun and Earth).NEOs have their own sub-types that depend on the risk level they represent to Earth.SummaryAsteroids can be classified by their composition and orbitThere are. Home / near Earth objects. Tag: near Earth objects. Posted in Civil China to launch near-Earth asteroid sample return mission in 2025. 2025 Septem. Posted in Civil Collection . Planetary Defense, Space Debris and Near-Earth Objects. With the increasing presence of space debris and the potential risk posed by near-Earth objects (NEOsQuantification of Near-Earth Objects Between : An
ADS Google Scholar P. Michel, C. Froeschlé, The location of linear secular resonances for semimajor axes smaller than 2 au. Icarus 128(1), 230–240 (1997)Article ADS Google Scholar P. Michel, F. Migliorini, A. Morbidelli, V. Zappala, The population of mars-crossers: classification and dynamical evolution. Icarus 145(2), 332–347 (2000)Article ADS Google Scholar A. Milani, A. Cellino, Z. Knežević, B. Novaković, F. Spoto, P. Paolicchi, Asteroid families classification: exploiting very large datasets. Icarus 239, 46–73 (2014). ADS Google Scholar A. Morbidelli, Origin and evolution of near earth asteroids, in Impact of Modern Dynamics in Astronomy. ed. by J. Henrard, S. Ferraz-Mello (Springer, Netherlands, Dordrecht, 1999), pp.39–50Chapter Google Scholar A. Morbidelli, M. Moons, Secular resonances in mean motion commensurabilities: the 2/1 and 3/2 cases. Icarus 102(2), 316–332 (1993)Article ADS Google Scholar A. Morbidelli, D. Nesvorný, Numerous weak resonances drive asteroids toward terrestrial planets orbits. Icarus 139(2), 295–308 (1999). ADS Google Scholar A. Morbidelli, W. Bottke, C. Froeschlé, P. Michel, et al. Origin and evolution of near-earth objects. Asteroids iii, 409 (2002)B. Novaković, C. Maurel, G. Tsirvoulis, Z. Knežević, Asteroid secular dynamics: Ceres’fingerprint identified. Astrophys. J. Lett. 807(1), L5 (2015)Article ADS Google Scholar C. Nugent, Detection of semimajor axis drifts in 54 near-earth asteroids: new measurements of the yarkovsky effect. Astron. J. (2012). Google Scholar D.P. O’Brien, R. Greenberg, The collisional and dynamical evolution of the main-belt and nea size distributions. Icarus 178(1), 179–212 (2005)Article ADS Google Scholar E. Perozzi, B. Borgia, M. Micheli, The european neo coordination centre. Mem. della Soc. Astron. Ital. 87,Comments
NASA's top expert on near-Earth objects says that new telescope systems, including a "last alert" system that's just now being set up, are gradually getting a handle on potentially threatening asteroids. But comets? That's a completely different story."We can do something about asteroids. Comets are a problem," said Donald Yeomans, the head of the Near-Earth Object Program at NASA's Jet Propulsion Laboratory in Pasadena, Calif.Yeomans is the author of "Near-Earth Objects: Finding Them Before They Find Us," a new book sizing up the cosmic perils posed by asteroids and comets — and looking ahead to the potential they offer for scientific discovery and economic exploitation.For an example of the perils, you need look no further than the dinosaurs — or, more accurately, the lack thereof. Scientists believe an asteroid impact along the coast of Mexico's Yucatan Peninsula set off a chain of events that killed off the dinosaurs and many other species 65 million years ago. A much smaller impact in 1908 blew down half a million acres' worth of trees in Siberia, and could have leveled a city nearly the size of Tokyo if its trajectory were different.Donald Yeomans is manager of Near Earth Object Program Office.NASA / JPL-Caltech"Near-Earth Objects" focuses on the peril and the potential of asteroids and comets.Princeton U. PressMore recently, astronomers have sounded a series of alerts over close encounters with passing asteroids — including three cases involving the asteroids 2012 DA14, 2011 AG5 and Apophis. It turns out that none of those space rocks will hit us in the foreseeable future, but 2012 DA14 is due to come within 13,000 miles on Feb. 15. That's closer than the orbits for geosynchronous satellites. And experts agree it's only a matter of time before astronomers find a large asteroid that's actually on a collision course.This is why Congress asked NASA in 1998 to identify 90 percent of the asteroids wider than a kilometer (0.6 miles). In 2011, NASA researchers declared that they achieved that goal. But they still have a long way to go to identify the smaller threats: The experts estimate that there are more than a million near-Earth asteroids capable of causing damage on the scale of 1908's Siberian fireball.Several projects are in the works to catalog those smaller asteroid threats, including some projects that are funded by NASA's observation program for near-Earth objects, which is allocated more than $20 million annually. One such program — known as the Asteroid Terrestrial-impact Last Alert System, or ATLAS — started receiving NASA funding just this month. The $5 million, five-year effort calls for building telescopes in Hawaii that could provide advance warning for the kinds of asteroids that have eluded bigger detection programs."We think it's possible
2025-04-11Georgina RannardClimate and science reporterGetty ImagesA large asteroid known as 2024 YR4 has grabbed headlines this week as scientists first raised its chances of hitting earth, then lowered them.The latest estimate says the object has a 0.28% chance of hitting Earth in 2032, significantly lower than the 3.1% chance earlier in the week.Scientists say it is now more likely to smash into the Moon, with Nasa estimating the probability of that happening at 1%.But in the time since 2024 YR4 was first spotted through a telescope in the desert in Chile two months ago, tens of other objects have passed closer to Earth than the Moon, which in astronomical terms sounds like a near miss.It is likely that others, albeit much smaller, have hit us or burned up in the atmosphere but gone unnoticed.This is the story of the asteroids that you never hear about – the fly-bys, the near-misses and the direct hits. The vast majority are harmless. But some carry the most valuable clues for unlocking mysteries in our universe, information we are desperate to get our hands on.Drs. Bill and Eileen Ryan, Magdalena Ridge Observatory 2.4m Telescope, New Mexico Tech2024 YR4 was first detected in December and there is small chance it could hit Earth on 22 December 2032Asteroids, also sometimes called minor planets, are rocky pieces left over from the formation of our solar system about 4.6 billion years ago.Rocks routinely orbit close to Earth, pushed by the gravity of other planets. For most of human history, it has been impossible to know how close we have come to being struck by a large asteroid. Serious monitoring of objects near Earth only started in the late 20th century, explains Professor Mark Boslough from the University of New Mexico. "Before that we were blissfully oblivious to them," he says.We now know that quite large objects - 40m across or more - pass between Earth and the Moon several times a year. That's the same size of asteroid that exploded over Siberia in 1908 injuring people and damaging buildings over 200 square miles.The most serious near-miss, and the closest comparison with YR4, was an asteroid called Apophis which was first spotted in 2004 and measured 375 meters across, or around the size of a cruise ship.Professor Patrick Michel from French National Centre for Scientific Research (CNRS) tracked Apophis and recalls it was considered the most hazardous asteroid ever detected.It took until 2013 to get enough observations to understand that it was not going to hit Earth.But he says there was one big difference with YR4. "We didn't know what to do. We discovered something, we determined an impact probability, and then thought, who do we call?" he says. Scientists and governments had no idea how to respond, he says.A large asteroid strike could be catastrophic if it hits an area where humans live. We don't know exactly how big YR4 is yet, but if it is at the top end of estimates, about 90m across, it would likely
2025-04-12Or different from an electrical interaction? Explain. Tutorials in JntroducJOry Physics McDennott, Shaffer, & P.E.G., U. Wash. ©Prentice Hall, Inc. First Edition, 2002 Magnets and magnetic fields EM 115 II. Magnetic fields We have observed that magnets interact even when they are not in direct contact. In electrostatics we used the idea of an electric field to account for the interaction between charges that were separated from one another. For magnetic interactions, we similarly define a magnetic field. A. Obtain a compass from a tutorial instructor. 1. Use the compass to explore the region around a bar magnet. Describe the behavior of the compass needle both near the poles of the magnet and in the region between the poles. To which class of objects from section I does the compass needle belong? Explain. 2. Move the compass far away from all other objects. Shake the compass and describe the behavior of the compass needle. Does the needle behave as if it is in a magnetic field? We can account for the behavior of the compass needle by supposing that it interacts with the Earth and that the Earth belongs to one of the categories from section I. To which class of objects from section I do your observations suggest the Earth belongs? Explain how you can tell. 3. We define the north pole of a magnet as the end that points toward the arctic region of the Earth when the magnet is free to rotate and is not interacting with
2025-03-29Massive 800-foot asteroid closely past the Earth. (Credit- Freepik)A huge stadium-sized space rock, the Asteroid 2023 SP1 cruised towards the Earth at a close distance today, NASA has confirmed. Asteroids, the rocky remnants of our solar system's formation, have left a deep mark on Earth in the form of craters, some colossal, some barely appearing on the landscape. These craters tell stories of scary collisions. Smaller asteroids, mere pebbles in the cosmic game, create fleeting streaks of light as meteors before burning up in our atmosphere. These leave behind no permanent mark, except for the occasional meteorite, a piece that survives the fiery destruction. Thankfully, the massive 800-foot asteroid escaped the Earth. Here is what NASA has revealed.Asteroid 2023 SP1: Key CharacteristicsAccording to NASA CNEOs data, this 800-foot extremely massive stadium-sized near-Earth object travelled towards Earth at a furious speed of 42480 kilometres per hour. The space rock made its closest approach to Earth today, February 7, 2024, passing at a close distance of a mere 3.41 million miles. And yes, the Asteroid 2008 OS7 was classified as a Potentially Hazardous Asteroid (PHA) by NASA's Center for Near-Earth Object Studies (CNEOS) due to its huge size and close approach towards the Earth.Asteroids and their potential to impact EarthMassive asteroids have played a significant role in shaping the history of Earth, both in terms of geological processes and the evolution of life. These celestial bodies, often remnants from the early solar system, are composed of rock, metal, and other materials. While most asteroids are relatively small and orbit the Sun within the asteroid belt between Mars and Jupiter, there is a potential threat posed by larger asteroids that could collide with Earth. Their impact on Earth has the potential to cause catastrophic consequences.The potential risk of a massive asteroid impact remains a concern, and ongoing research and preparedness are crucial to understanding and mitigating this potential threat. Advances in technology and international collaboration will continue to play a vital role in monitoring and responding to the ever-present cosmic hazards that our planet faces.
2025-04-04Sisto, A. Brunini, L.D. Dirani, R.B. Orellana, Hilda asteroids among Jupiter family comets. Icarus 174(1), 81–89 (2005)Article ADS Google Scholar P. Farinella, C. Froeschlé, C. Froeschlé, R. Gonczi, G. Hahn, A. Morbidelli, G.B. Valsecchi, Asteroids falling into the sun. Nature 371(6495), 314–317 (1994)Article ADS Google Scholar J.A. Fernández, T. Gallardo, A. Brunini, Are there many inactive Jupiter-family comets among the near-earth asteroid population? Icarus 159(2), 358–368 (2002)Article ADS Google Scholar J.A. Fernández, T. Gallardo, A. Brunini, Are there many inactive Jupiter-family comets among the near-earth asteroid population? Icarus 159(2), 358–368 (2002). ADS Google Scholar J.A. Fernández, A. Sosa, T. Gallardo, J.N. Gutiérrez, Assessing the physical nature of near-earth asteroids through their dynamical histories. Icarus 238, 1–12 (2014). ADS Google Scholar T. Gallardo, Atlas of the mean motion resonances in the solar system. Icarus 184(1), 29–38 (2006). ADS Google Scholar B.J. Gladman, F. Migliorini, A. Morbidelli, V. Zappala, P. Michel, A. Cellino, C. Froeschle, H.F. Levison, M. Bailey, M. Duncan, Dynamical lifetimes of objects injected into asteroid belt resonances. Science 277(5323), 197–201 (1997)Article ADS Google Scholar B. Gladman, P. Michel, C. Froeschlé, The near-earth object population. Icarus 146(1), 176–189 (2000)Article ADS Google Scholar M. Granvik, A. Morbidelli, R. Jedicke, B. Bolin, W.F. Bottke, E. Beshore, D. Vokrouhlickỳ, M. Delbò, P. Michel, Super-catastrophic disruption of asteroids at small perihelion distances. Nature 530(7590), 303–306 (2016)Article ADS Google Scholar M. Granvik, A. Morbidelli, D. Vokrouhlickỳ, W.F. Bottke, D. Nesvornỳ, R. Jedicke, Escape of asteroids from the main belt. Astron. Astrophys. 598, A52 (2017)Article ADS
2025-03-30