Live tracking — NASA NeoWs

Next: (2017 RO17)

Next close approach: (2017 RO17) on Oct 13, 2026 — today, about 26 m across, passing at 30,080,211 km (78 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 — and the closest passes this week are still millions of kilometres away. You see “close approaches” 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 — or in the wider catalog — 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 “close” 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)NameDiameterMiss DistanceSpeedStatus
Oct 13, 2026, 00:10 UTC(2017 RO17)16–36 m
30,080,211 km
78 LD
30,403 km/hRoutine pass
Oct 13, 2026, 01:33 UTC339714 (2005 ST1)226–506 m
20,334,583 km
53 LD
51,396 km/hRoutine pass
Oct 13, 2026, 04:16 UTC(2012 WH1)38–86 m
15,346,503 km
40 LD
25,052 km/hRoutine pass
Oct 13, 2026, 16:48 UTC(2015 TG24)12–27 m
28,182,879 km
73 LD
57,591 km/hRoutine pass
Oct 13, 2026, 16:53 UTC(2016 TG56)53–119 m
70,040,598 km
182 LD
55,520 km/hRoutine pass
Oct 13, 2026, 18:52 UTC(2011 UH20)160–358 m
41,396,652 km
108 LD
87,598 km/hPHA — monitored
Oct 13, 2026, 19:42 UTC(2010 DO)124–277 m
23,042,474 km
60 LD
91,054 km/hPHA — monitored
Oct 14, 2026, 05:02 UTC(2016 UZ41)229–513 m
29,796,273 km
77 LD
54,978 km/hRoutine pass
Oct 14, 2026, 05:49 UTC(2018 EH4)123–275 m
8,427,648 km
22 LD
47,601 km/hPHA — monitored
Oct 14, 2026, 05:49 UTC678976 (2018 EH4)123–274 m
8,427,728 km
22 LD
47,601 km/hPHA — monitored
Oct 14, 2026, 23:14 UTC(2019 SB1)271–605 m
37,592,118 km
98 LD
80,832 km/hRoutine pass
Oct 15, 2026, 02:57 UTC(2009 TK8)246–550 m
12,187,273 km
32 LD
53,681 km/hRoutine pass
Oct 15, 2026, 08:22 UTC(2017 TM6)58–130 m
58,678,323 km
153 LD
56,055 km/hRoutine pass
Oct 15, 2026, 20:32 UTC(2013 JR22)178–398 m
18,290,738 km
48 LD
75,524 km/hRoutine pass
Oct 16, 2026, 03:23 UTC(2000 SZ162)9–21 m
7,622,018 km
20 LD
20,486 km/hRoutine pass
Oct 16, 2026, 03:29 UTC(2015 HH10)0.6–1.4 km
64,935,264 km
169 LD
75,214 km/hRoutine pass
Oct 16, 2026, 03:34 UTC(2020 QG3)152–339 m
8,244,155 km
21 LD
36,517 km/hPHA — monitored
Oct 16, 2026, 03:34 UTC679786 (2020 QG3)152–339 m
8,244,146 km
21 LD
36,517 km/hPHA — monitored
Oct 16, 2026, 16:58 UTC(2015 XN128)31–69 m
59,500,842 km
155 LD
5,875 km/hRoutine pass
Oct 17, 2026, 01:39 UTC144900 (2004 VG64)0.6–1.3 km
26,873,815 km
70 LD
80,990 km/hPHA — monitored
Oct 17, 2026, 03:03 UTC(2005 VS)95–212 m
15,738,548 km
41 LD
24,090 km/hRoutine pass
Oct 17, 2026, 04:02 UTC(2008 TC4)124–278 m
45,552,721 km
118 LD
90,045 km/hPHA — monitored
Oct 17, 2026, 04:02 UTC614134 (2008 TC4)124–278 m
45,552,721 km
118 LD
90,045 km/hPHA — monitored
Oct 17, 2026, 04:42 UTC(2014 JR24)4–8 m
65,155,068 km
169 LD
60,072 km/hRoutine pass
Oct 17, 2026, 09:33 UTC(2002 TH68)120–269 m
73,549,238 km
191 LD
69,791 km/hRoutine pass
Oct 17, 2026, 10:29 UTC(2016 LC9)11–24 m
16,990,663 km
44 LD
13,007 km/hRoutine pass
Oct 17, 2026, 10:35 UTC(2018 PZ21)12–27 m
29,282,896 km
76 LD
42,636 km/hRoutine pass
Oct 17, 2026, 18:26 UTC(2015 HR11)175–391 m
26,601,231 km
69 LD
63,958 km/hPHA — monitored
Oct 17, 2026, 18:36 UTC(2016 TQ54)10–22 m
63,040,348 km
164 LD
79,139 km/hRoutine pass
Oct 17, 2026, 19:42 UTC(2017 MA4)0.5–1.1 km
70,436,910 km
183 LD
97,430 km/hRoutine pass

Source: NASA Center for Near-Earth Object Studies · NeoWs feed endpoint. 12 of these are flagged PHA (Potentially Hazardous Asteroid) — a monitoring designation, not an impact prediction.

What “Close Approach” Actually Means

In astronomy, “close” 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 — called one lunar distance, or 1 LD — 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 — 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 — the near-Earth asteroids, or NEAs — 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 “close approaches” (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 — 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 — 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 — 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 — usually after a few weeks of follow-up — 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 “Potentially Hazardous Asteroid” Really Means

The term Potentially Hazardous Asteroid, or PHA, is one of the most misread phrases in astronomy. It does not mean “going to hit Earth.” 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 — every one is being watched and every one is currently expected to miss Earth. The PHA label is best read as “keep monitoring,” 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 — 13 April 2029

About 340 metres across. On 13 April 2029, Apophis will pass at roughly 31,000 km from Earth — 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 — 15 February 2013

A roughly 20-metre object broke up over Russia at about 30 km altitude. It was not pre-detected — 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 — 30 June 1908

An airburst over Siberia, energy equivalent to roughly 15 megatons of TNT, flattened around 2,000 km² of forest. Best modern estimate of the object: a stony asteroid roughly 50–60 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 — “mini-moon” 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 “wandering stars” — Sun, Moon, Mercury, Venus, Mars, Jupiter, Saturn — 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 “an asteroid is approaching, therefore X will happen.” The idea that close approaches are spiritual events is a recent social-media exaggeration, not a part of the tradition. If you see an “asteroid warning” 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 — sign, house, aspect — 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.

“NASA is hiding an asteroid that will hit us.”

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 — 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.

“Astrologers can predict asteroid impacts.”

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 — work done by JPL and a handful of other groups. Astrology has never claimed and cannot perform this work.

“Every close approach is dangerous.”

No. Close in astronomy means tens of thousands to millions of kilometres. The default outcome of a close approach is “it passes by and you do not notice.” A pass under 1 lunar distance is rare and newsworthy; everything beyond that, in honest framing, is routine.

“Asteroid X is named after me and that means something for my life.”

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.

For watching close approaches from home: passes brighter than magnitude +11 are reachable with a backyard 8″ 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 (2017 RO17) on Oct 13, 2026 — today. It will pass Earth at a miss distance of 30,080,211 km (78 LD). For context, the Moon is about 384,400 km away, so this asteroid passes 78 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 — 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 — 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 — 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 — 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 — 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 — 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.

This page is editorial. Live data comes from NASA NeoWs. The astrology framing is honest tradition — asteroids are interesting astronomy, not predictive astrology. See our AI disclosure for editorial standards.