C/2026 A1 (MAPS)

Kreutz sungrazer comet From Wikipedia, the free encyclopedia

C/2026 A1 (MAPS), formerly known by its temporary designation as 6AC4721, is a Kreutz sungrazer comet discovered on 13 January 2026 from the AMACS1 Observatory in the Atacama Desert. This comet was discovered through the MAPS program [fr], which was led by Alain Maury, Georges Attard [fr], Daniel Parrott and Florian Signoret.[b] On 4 April 2026, it will pass about 162,000 km (101,000 mi) from the surface of the Sun.[a] When near the Sun, the forward scattering of light could make the comet significantly brighter,[12] but hard to see against the glare of the Sun.[c] How bright the comet will get is largely unknown as it depends on the comet's survival upon perihelion approach.

DiscoveredbyMAP Observation Program [fr]
Discoverydate13 January 2026
6AC4721, CK26A010
Quick facts Discovery, Discovered by ...
C/2026 A1 (MAPS)
Comet MAPS as seen by the James Webb Space Telescope on 7 February 2026
Discovery[1][2]
Discovered byMAP Observation Program [fr]
Discovery siteAMACS1, Chile (W94)
Discovery date13 January 2026
Designations
6AC4721, CK26A010
Orbital characteristics[3]
Epoch10 February 2026
(JD 2461081.5)
Observation arc66 days
Earliest precovery date18 December 2025[4]
Number of
observations
954[5]
Orbit typeKreutz sungrazer
Aphelion308±2 AU
Perihelion0.005732 AU (1.233 R)[a]
Semi-major axis154±1 AU
Eccentricity0.99996
Orbital period1911±14 years
1703 years (inbound)[6]
Max. orbital speed556 km/s[7]
Inclination144.49°
7.86°
Argument of
periapsis
86.3°
Mean anomaly359.97°
Next perihelion4 April 2026 ≈14:23 UT[7]
TJupiter–0.043
Earth MOID0.556 AU
Jupiter MOID2.987 AU
Physical characteristics[3]
Mean radius
0.2 km (0.12 mi)[8]
Comet total
magnitude
(M1)
14.8±1
9.7
(20 March 2026)[9]
Close

Observational history

C/2026 A1 imaged by Alain Maury and Georges Attard on 17 January 2026

C/2026 A1 (MAPS) was discovered from the AMACS1 Observatory at San Pedro de Atacama, using a 0.28 m (11 in) f/2.2 Schmidt telescope with a CCD camera.[1] It was discovered at a distance of 2.056 AU (307.6 million km; 191.1 million mi) from the Sun, making it the furthest Kreutz sungrazer ever discovered,[13] surpassing the record previously held by Comet Ikeya–Seki,[d] allowing a lead time of observations for approximately 81 days before perihelion.[15]

The comet was 17.8 magnitude at the moment of discovery and was located in the constellation Columba.[1]

Earliest precovery date is December 2025, when it was about magnitude 20.[4] Its discovery was officially announced on 20 January 2026.[1][2] It is expected to become visible in 8 to 10-inch telescopes by late March, a few days before perihelion.[16][17] By mid March it had brightened to an apparent magnitude of about 10.[9] It will cross the celestial equator on 30 March 2026.[18] Due to its relatively low declination in the sky relative to the Sun, it will become more favorable to view from the Southern hemisphere than in the north.[16]

As seen from Earth, the comet will come to solar conjunction on 4 April 2026 around 13:20 (behind the Sun) and 15:36 UT (in front of the Sun).[19] For both, it will be 0.04 degrees from the center of the Sun (the Sun has a width of 0.5 degrees).[19] It is expected to enter SOHO–LASCO's field-of-view by 2 April 2026.[20]

Orbit

C/2026 A1 is a Kreutz group comet. It was initially thought to belong to the Pe subgroup, a subgroup of the Kreutz Sungrazers closely associated with subgroup I, which all fragmented from the Great Comet of 1106.[21] This specific subgroup include some bright members like the Great Comet of 1843 and C/1963 R1 (Pereyra).[22][e] However, its extraordinarily long orbital period suggested it's only a coincidence and it may possibly be a member of a yet-unknown distinct subgroup instead.[23]

It will pass through the solar corona and reach perihelion on 4 April 2026 around 14:23 UT when it will be 0.005732 AU (1.233 R) from the center of the Sun[7] or about 162,000 km from the surface of the Sun.[a] There is no chance of a solar impact as the 5-sigma uncertainty is only ±2000 km,[3][f] giving a minimum possible approach of about 160000 km. It will then make closest approach to Earth the next day around 5 April 2026 23:59 UT when it will be 0.961 AU (143.8 million km) from Earth.[24]

With an observation arc of 66 days, the comet's inbound orbital period (calculated at epoch 1800, which is before entering the planetary region of the Solar System) suggests it last reached perihelion around 1700 years ago,[6] suggesting that it may be a second-generation fragment from the Great Comet of 371 BC itself,[23] specifically the comet of 363 AD that was witnessed by Ammianus Marcellinus.[25]

Physical characteristics

In January 2026, initial estimates of the upper limit for the size of its nucleus placed it at less than 2.4 km (1.5 mi) in diameter.[16][26] A study published in March 2026 using the data from the James Webb Space Telescope (JWST) concluded that the comet is roughly 400 m (1,300 ft) in diameter,[8] about the size of C/2011 W3 (Lovejoy),[27] however its authors noted that the comparison has to be treated with caution as C/2026 A1 is the only Kreutz comet that we have direct measurements of its nucleus out of the more than 5,000 members of the family we had known so far.[8]

See also

Notes

  1. The comet will pass 0.005732 AU (1.233 R) from the center of the Sun[7] which is (0.233 solar radii * 695700 km) = 162,000 km (101,000 mi) from the surface of the Sun.
  2. C/2026 A1 is the third comet discovered by the program after C/2025 L2 (MAPS)[10] and C/2025 O2 (MAPS)[11]
  3. Observing a comet when it is very close to the Sun can be dangerous.
  4. Comet Ikeya–Seki was first discovered at a distance of 1.11 AU (166 million km) from the Sun on 18 September 1965,[14] which gave astronomers approximately 33 days to observe the comet inbound.[15]
  5. The Great Comet of 1843 passed 132000 km from the surface of the Sun and C/1963 R1 (Pereyra) passed 56000 km from the surface of the Sun. With a short observation arc of 8 days, the Kreutz Great Southern Comet of 1887 is believed to have passed about 27000 km from the surface of the Sun. Sun-plunger (with a sun-striking trajectory and non-Kreutz member) C/2007 M5 (SOHO), if it did not get vaporized by the extreme solar radiation and tidal forces, would have tried to impact the Sun at 0.0011 AU (160 thousand km; 100 thousand mi) from the Sun's center.
  6. JPL #8 at the JPL SBDB shows a 1-sigma uncertainty of 2.6E-6 AU which is a 1-sigma uncertainty of 389 km or a 5-sigma uncertainty of 2000 km (2.6E-6 * AU * 5).

References

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