Live tracking โ NASA NeoWs
Next: (2019 MH1)
Next close approach: (2019 MH1) on Aug 25, 2026 โ today, about 49 m across, passing at 54,786,652 km (142 LD).
Data: NASA NeoWs feed. Page rebuilds every 6 hours. None of these asteroids are on a collision course with Earth.
Asteroid Tracker: Next Near-Earth Asteroids From NASA
Is an asteroid going to hit Earth this week? No. NASA tracks every asteroid that comes anywhere near our orbit โ and the closest passes this week are still millions of kilometres away. You see โclose approachesโ in the news because we now have very good telescopes, not because impacts are imminent. The table below shows the next seven catalogued passes, pulled live from NASA's NeoWs feed.
Is an Asteroid Going to Hit Earth This Week?
No. Every asteroid currently tracked by NASA, JPL, ESA, and the world's observatories has a calculated future trajectory, and none of the objects on this page โ or in the wider catalog โ are on a collision course with Earth in the next 100 years. The reason close approaches make the news is the combined effect of three things: there are millions of small bodies in the inner solar system, modern survey telescopes catch almost every one that comes within Earth's neighbourhood, and astronomical โcloseโ routinely means millions of kilometres away.
If a real impact threat were ever identified, agencies would issue formal public warnings through the UN Office for Outer Space Affairs and the International Asteroid Warning Network. As of today, no such warning is active anywhere in the world.
Upcoming Close Approaches (Next 7 Days)
Sorted by approach date. Miss distance is the asteroid's closest distance to Earth's centre. For reference, the Moon orbits Earth at about 384,400 km (1 lunar distance, abbreviated LD).
| Date (UTC) | Name | Diameter | Miss Distance | Speed | Status |
|---|---|---|---|---|---|
| Aug 25, 2026, 00:04 UTC | (2019 MH1) | 30โ68 m | 54,786,652 km 142 LD | 82,707 km/h | Routine pass |
| Aug 25, 2026, 06:59 UTC | (2005 EY169) | 93โ207 m | 62,610,526 km 163 LD | 40,833 km/h | Routine pass |
| Aug 25, 2026, 08:45 UTC | (2019 GJ4) | 17โ37 m | 50,210,606 km 131 LD | 52,857 km/h | Routine pass |
| Aug 25, 2026, 09:58 UTC | (2016 XJ) | 9โ20 m | 59,946,801 km 156 LD | 20,056 km/h | Routine pass |
| Aug 25, 2026, 12:42 UTC | (2019 GV5) | 4โ8 m | 31,170,093 km 81 LD | 21,246 km/h | Routine pass |
| Aug 25, 2026, 19:45 UTC | (2019 DN1) | 5โ10 m | 65,395,170 km 170 LD | 57,776 km/h | Routine pass |
| Aug 26, 2026, 04:12 UTC | (2018 TM3) | 3โ7 m | 60,112,640 km 156 LD | 58,092 km/h | Routine pass |
| Aug 26, 2026, 16:35 UTC | 66146 (1998 TU3) | 3.6โ8.0 km | 13,506,722 km 35 LD | 40,709 km/h | Routine pass |
| Aug 26, 2026, 22:14 UTC | (2019 CE5) | 55โ122 m | 57,265,569 km 149 LD | 24,349 km/h | Routine pass |
| Aug 27, 2026, 02:01 UTC | 523609 (2005 PJ2) | 330โ738 m | 7,077,379 km 18 LD | 81,899 km/h | PHA โ monitored |
| Aug 27, 2026, 03:12 UTC | (2005 QQ87) | 72โ161 m | 20,672,081 km 54 LD | 73,280 km/h | Routine pass |
| Aug 27, 2026, 03:43 UTC | (2017 WJ16) | 34โ77 m | 39,639,327 km 103 LD | 16,663 km/h | Routine pass |
| Aug 27, 2026, 11:59 UTC | (2002 GQ5) | 180โ402 m | 16,819,931 km 44 LD | 49,404 km/h | Routine pass |
| Aug 27, 2026, 11:59 UTC | 612346 (2002 GQ5) | 173โ387 m | 16,819,881 km 44 LD | 49,404 km/h | Routine pass |
| Aug 27, 2026, 17:51 UTC | (2013 VJ11) | 7โ16 m | 13,745,154 km 36 LD | 26,710 km/h | Routine pass |
| Aug 27, 2026, 21:47 UTC | (2019 QF2) | 73โ163 m | 58,346,530 km 152 LD | 73,102 km/h | Routine pass |
| Aug 28, 2026, 00:31 UTC | (2019 NC1) | 139โ312 m | 46,139,345 km 120 LD | 44,848 km/h | Routine pass |
| Aug 28, 2026, 10:34 UTC | (2016 PP39) | 77โ171 m | 45,742,161 km 119 LD | 27,392 km/h | Routine pass |
| Aug 28, 2026, 15:47 UTC | 221455 (2006 BC10) | 332โ741 m | 3,584,833 km 9.3 LD | 68,412 km/h | PHA โ monitored |
| Aug 28, 2026, 23:43 UTC | (2017 BP31) | 286โ640 m | 4,278,975 km 11 LD | 73,621 km/h | PHA โ monitored |
| Aug 28, 2026, 23:55 UTC | (2017 DR37) | 110โ245 m | 68,191,142 km 177 LD | 48,522 km/h | Routine pass |
| Aug 29, 2026, 15:12 UTC | (2020 DX1) | 13โ30 m | 16,511,204 km 43 LD | 24,546 km/h | Routine pass |
| Aug 30, 2026, 17:12 UTC | 485823 (2012 DF61) | 201โ449 m | 45,892,005 km 119 LD | 39,626 km/h | Routine pass |
| Aug 30, 2026, 17:37 UTC | (2007 EK) | 4โ8 m | 4,188,706 km 11 LD | 32,907 km/h | Routine pass |
| Aug 30, 2026, 18:51 UTC | (2012 TB53) | 64โ143 m | 28,836,716 km 75 LD | 28,687 km/h | Routine pass |
| Aug 30, 2026, 19:37 UTC | (2019 GK5) | 221โ494 m | 26,507,432 km 69 LD | 45,467 km/h | Routine pass |
| Aug 30, 2026, 22:14 UTC | (2012 LE11) | 0.6โ1.4 km | 26,064,307 km 68 LD | 36,259 km/h | Routine pass |
| Aug 30, 2026, 23:24 UTC | (2013 JR28) | 121โ272 m | 39,176,126 km 102 LD | 52,868 km/h | PHA โ monitored |
| Aug 31, 2026, 01:25 UTC | (2007 PB8) | 142โ318 m | 31,128,825 km 81 LD | 42,381 km/h | Routine pass |
| Aug 31, 2026, 01:38 UTC | (2008 HU4) | 6โ13 m | 15,969,004 km 42 LD | 6,794 km/h | Routine pass |
Source: NASA Center for Near-Earth Object Studies ยท NeoWs feed endpoint. 5 of these are flagged PHA (Potentially Hazardous Asteroid) โ a monitoring designation, not an impact prediction.
What โClose Approachโ Actually Means
In astronomy, โcloseโ is not the same word that humans use day-to-day. A close approach in NASA's catalog usually means the asteroid passes within a few million kilometres of Earth's orbit. For comparison: the Moon, which is the brightest object in the night sky, orbits Earth at an average distance of 384,400 kilometres. That distance โ called one lunar distance, or 1 LD โ is the unit astronomers use when they want to give a sense of how genuinely close a pass is.
Most of the asteroids in the table above pass tens to hundreds of lunar distances from Earth. A pass at 10 LD is already 3.8 million kilometres away โ far enough that no telescope on Earth except the largest professional instruments will pick the object up. A pass under 1 LD is rare and newsworthy; a pass under 0.1 LD (about 38,000 km, inside the orbit of geostationary satellites) is rarer still and is the level at which agencies start putting out educational press notes.
If a real impact threat ever emerged, NASA, ESA, and the UN Office for Outer Space Affairs would issue advance public warnings through formal channels. As of now, no such warning is active. Every asteroid on this page passes harmlessly.
Why So Many Asteroids?
The inner solar system is unimaginably crowded. There are several million asteroids larger than a kilometre across in the main belt between Mars and Jupiter, and tens of millions smaller. A subset of them โ the near-Earth asteroids, or NEAs โ have orbits that bring them inside Earth's neighbourhood. NASA currently has roughly 30,000+ NEAs catalogued, with hundreds more added every month by ground-based surveys.
Because of this density, the expected baseline rate of โclose approachesโ (objects passing within about 0.05 AU, or 7.5 million km) is on the order of 100 per week. Most are small objects you would never have heard of without modern telescopes. The numbers feel alarming if you read them without context โ but they describe the routine background of the inner solar system, not a recent change in risk.
If anything, the rising number reflects better monitoring. Pan-STARRS, Catalina Sky Survey, and ATLAS together cover the whole sky every few nights, down to objects the size of a school bus. Twenty years ago we missed nearly all of them. Today we catch almost everything larger than 50 metres โ and we are getting steadily better at catching smaller ones.
How NASA Tracks Asteroids
Asteroid tracking is a multi-stage pipeline. New objects are discovered by automated survey telescopes โ chiefly the Catalina Sky Survey in Arizona, the Pan-STARRS array in Hawaii, and the ATLAS network on Hawaii and elsewhere. These telescopes scan large fields of sky every clear night, software flags anything that has moved between exposures, and the candidate detections are reported to the IAU's Minor Planet Center.
Once an object is confirmed, follow-up observations from professional observatories and a worldwide amateur network nail down its orbit. The data feeds into NASA's JPL Small-Body Database and the Center for Near-Earth Object Studies (CNEOS), which runs the Sentry impact monitoring system. Sentry continuously projects each asteroid's orbit forward 100+ years and computes an impact probability for every plausible future close pass. When the orbital uncertainty shrinks โ usually after a few weeks of follow-up โ most candidates drop off the watch list entirely.
Space-based assets contribute too. NEOWISE, the infrared follow-up to the WISE mission, has discovered hundreds of NEAs. The upcoming NEO Surveyor infrared space telescope, planned for launch in 2027, is designed specifically to find the dark NEAs that ground-based optical surveys miss.
What โPotentially Hazardous Asteroidโ Really Means
The term Potentially Hazardous Asteroid, or PHA, is one of the most misread phrases in astronomy. It does not mean โgoing to hit Earth.โ It is a NASA monitoring classification with two precise criteria:
- Estimated diameter of at least 140 metres.
- Minimum orbital intersection distance with Earth of 0.05 AU (about 7.5 million km) or less.
Both conditions have to be met together. An asteroid that is large enough but never comes close, or one that comes close but is too small to do regional damage, is not a PHA. The classification simply identifies the objects worth monitoring carefully because their orbits could, on long timescales, evolve into impact trajectories.
There are roughly 2,400 PHAs currently catalogued. None of them have a meaningful impact probability in the next century โ every one is being watched and every one is currently expected to miss Earth. The PHA label is best read as โkeep monitoring,โ not as a forecast.
Famous Past (And Future) Close Approaches
A few asteroids have entered popular memory either because they came genuinely close, or because they actually arrived.
99942 Apophis โ 13 April 2029
About 340 metres across. On 13 April 2029, Apophis will pass at roughly 31,000 km from Earth โ closer than geostationary satellites and visible to the naked eye from parts of Africa, Europe, and Asia. This is the closest predicted pass by an object of its size in the modern catalog. NASA, ESA, and JAXA all confirm no impact risk for at least the next 100 years.
Chelyabinsk meteor โ 15 February 2013
A roughly 20-metre object broke up over Russia at about 30 km altitude. It was not pre-detected โ too small for the surveys of the time, and approaching from the direction of the Sun where telescopes cannot look. The shockwave shattered windows across Chelyabinsk Oblast, injuring about 1,500 people; there were no direct fatalities. Modern surveys have closed much of the gap that allowed this object to arrive unseen.
Tunguska event โ 30 June 1908
An airburst over Siberia, energy equivalent to roughly 15 megatons of TNT, flattened around 2,000 kmยฒ of forest. Best modern estimate of the object: a stony asteroid roughly 50โ60 metres across. No human deaths were recorded (the region was almost uninhabited), but a similar event over a populated area today would be a regional disaster. June 30, the anniversary, is now observed as International Asteroid Day.
2024 PT5 โ โmini-moonโ of 2024
A small asteroid temporarily captured by Earth's gravity for about two months in late 2024, briefly becoming a second natural satellite of Earth before continuing on its solar orbit. About 10 metres across, far too small to be a hazard, but a vivid demonstration of how dynamic the near-Earth population is.
None of these are imminent. They are listed here as context for how the catalog actually behaves over decades.
Asteroids in Astrology Tradition
Classical Western astrology does not track asteroids. The system was built on the seven visible โwandering starsโ โ Sun, Moon, Mercury, Venus, Mars, Jupiter, Saturn โ and was extended only slowly to include Uranus, Neptune, Pluto, and a small handful of bodies after they were discovered. The asteroids that are used by modern astrologers form a short list: the four major asteroids Ceres, Pallas, Juno, and Vesta (all discovered in the early 1800s), plus the centaur Chiron and occasionally a few other named bodies like Eros or Psyche.
Mainstream astrology does not read newly-discovered or incoming asteroids as omens. There is no traditional doctrine that says โan asteroid is approaching, therefore X will happen.โ The idea that close approaches are spiritual events is a recent social-media exaggeration, not a part of the tradition. If you see an โasteroid warningโ framed as astrological prediction, it is invented framing.
Where asteroids do enter serious astrological work, they are treated like any other symbolic body in a birth chart โ sign, house, aspect โ and read as a thematic addition to the core seven. Chiron, the most widely used, points to a place of wounding and healing. Ceres maps onto nurture and grief. The honest astrological position on near-Earth asteroids is: interesting astronomy, not predictive astrology.
What Asteroid Tracking Does Not Mean
Asteroid news travels fast and gets twisted on the way. The following claims are common online and are not supported.
โNASA is hiding an asteroid that will hit us.โ
No. NASA publishes every catalogued close approach with the full miss distance, velocity, and orbital uncertainty on a public website. The JPL Small-Body Database and the Center for Near-Earth Object Studies are open APIs โ the same data this page is pulling. Astronomy is one of the most distributed and transparent sciences in the world; thousands of independent amateur and professional observers would notice an attempt to suppress an impact.
โAstrologers can predict asteroid impacts.โ
No. Astrology is a symbolic system, not a celestial-mechanics calculator. Impact prediction requires precise orbital determination, gravitational-perturbation modelling, and statistical analysis of many millions of trial trajectories โ work done by JPL and a handful of other groups. Astrology has never claimed and cannot perform this work.
โEvery close approach is dangerous.โ
No. Close in astronomy means tens of thousands to millions of kilometres. The default outcome of a close approach is โit passes by and you do not notice.โ A pass under 1 lunar distance is rare and newsworthy; everything beyond that, in honest framing, is routine.
โAsteroid X is named after me and that means something for my life.โ
No. Asteroids are named under conventions set by the International Astronomical Union, typically by the discoverer following a peer-reviewed naming process. The names follow rules about appropriate referents (no political figures still living, no commercial promotion, no profanity). They are not assigned with personal-spiritual meaning, and an asteroid sharing a name with you does not affect your chart.
How to Follow Asteroid News (Trusted Sources)
This page reads from NASA NeoWs on a 6-hour cycle. For real-time updates and authoritative orbital data, these are the primary feeds the rest of the field uses.
- NASA Center for Near-Earth Object Studies (CNEOS) โ the authoritative source for close-approach tables, the Sentry impact risk system, and the cumulative discovery statistics.
- IAU Minor Planet Center โ the international clearinghouse where every new asteroid observation is reported and confirmed.
- NASA NeoWs API โ the open feed that powers this page. Free, no auth beyond a free api.nasa.gov key for production use.
- ESA Planetary Defence Office โ the European Space Agency's parallel monitoring programme; runs the NEOCC risk list independently from NASA.
For watching close approaches from home: passes brighter than magnitude +11 are reachable with a backyard 8โณ telescope; the rare passes inside 1 lunar distance are sometimes naked-eye briefly. Sites like TheSkyLive and In-The-Sky.org publish live finder charts.
Frequently Asked Questions
When is the next asteroid close approach to Earth?
The next catalogued close approach is asteroid (2019 MH1) on Aug 25, 2026 โ today. It will pass Earth at a miss distance of 54,786,652 km (142 LD). For context, the Moon is about 384,400 km away, so this asteroid passes 142 LD farther than the Moon. It is not on a collision course.
How big does an asteroid have to be to count as "potentially hazardous"?
NASA classifies a near-Earth object as a Potentially Hazardous Asteroid (PHA) when it meets two criteria together: an estimated diameter of at least 140 metres, and an orbit that brings it within 0.05 astronomical units (about 7.5 million kilometres) of Earth's orbit. PHA is a monitoring classification โ it does not mean the asteroid will hit us. In modern history, no PHA has ever struck Earth.
Can NASA stop an asteroid from hitting Earth?
For small, late-detected asteroids, no โ there is currently no operational system that could intercept on short notice. For asteroids detected years in advance, yes: in September 2022, NASA's DART mission deliberately collided with the asteroid moonlet Dimorphos and measurably altered its orbit, the first kinetic-impact deflection test in history. The conclusion: given enough lead time, a small nudge applied years before an impact can move an asteroid by enough to miss Earth. The hard part is detection, not deflection.
What is the largest near-Earth asteroid?
1036 Ganymed, discovered in 1924, is the largest known near-Earth asteroid at roughly 38 kilometres across. It is too far from Earth's orbit to be classified as a PHA. Among PHAs, the largest are 4179 Toutatis (about 4.5 km) and 53319 (1999 JM8) at about 7 km โ neither poses a threat in the foreseeable future.
How fast do asteroids move when they pass Earth?
Typical relative velocities at close approach range from about 5 km/s to over 30 km/s, which is 18,000 to 108,000 kilometres per hour. The speed depends on the asteroid's orbit and how Earth's orbital motion adds to or subtracts from it. Fast head-on encounters tend to come from steeper orbits; slow flybys from orbits that closely match Earth's.
Has Earth ever been hit by a large asteroid?
In deep time, yes โ the Chicxulub impact 66 million years ago ended the non-avian dinosaurs. In recorded history, the largest confirmed events are Tunguska (1908, an airburst over Siberia from an object roughly 50 metres across) and Chelyabinsk (2013, a roughly 20-metre object that broke up over Russia, injuring about 1,500 people from shattered glass โ no fatalities). Both objects were small by PHA standards. Earth has not been hit by an asteroid larger than 50 metres in modern history.
Is asteroid Apophis going to hit Earth in 2029?
No. Asteroid 99942 Apophis will pass safely on 13 April 2029 at a miss distance of about 31,000 kilometres โ closer than geostationary satellites, but a clean miss. NASA, ESA, and JAXA all confirm there is no impact risk for at least the next 100 years. The 2029 flyby is, however, the closest predicted approach by an object of its size (about 340 metres) in the modern catalogue, and several space agencies plan rendezvous missions to study it.
Why does NASA track so many asteroids?
Because most asteroids are not yet catalogued. NASA estimates roughly 30,000 near-Earth asteroids are currently known and several million more remain undiscovered, mostly small. Tracking serves two purposes: building enough orbital data on each known object to rule out future impact, and using ground-based surveys (Pan-STARRS, Catalina, ATLAS) plus JPL's Sentry monitoring system to catch any new object as early as possible.
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This page is editorial. Live data comes from NASA NeoWs. The astrology framing is honest tradition โ asteroids are interesting astronomy, not predictive astrology. See our AI disclosure for editorial standards.