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2I/Borisov

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2I/Borisov
Borisov in October 2019[a]
Discovery
Discovered byGennadiy Borisov
Discovery siteMARGO observatory, Nauchnyy, Crimea
Discovery date30 August 2019
Earliest precovery:
13 December 2018
Orbital characteristics
Epoch5 January 2020[3]
Number of
observations		1191
Perihelion2.00662±0.00002 AU
Semi-major axis−0.85132±0.00007 AU[b]
Eccentricity3.3570±0.0002 (JPL)
3.357 (MPC)[4]
Inclination44.0535°±0.0001°
Last perihelion8 December 2019[3][4][5]
Earth MOID1.09302 AU
Jupiter MOID2.388 AU
Physical characteristics
Dimensions≤ 0.5 km[6](for an albedo of 0.04)
≤ 0.4 km[7]

2I/Borisov, originally designated C/2019 Q4 (Borisov),[8] is the first observed rogue comet and the second observed interstellar interloper after ʻOumuamua.[9][10] It was discovered by the Crimean amateur astronomer and telescope maker Gennadiy Borisov on 30 August 2019 UTC (29 August local time.)[11][12]

2I/Borisov has a heliocentric orbital eccentricity of 3.36 and is not bound to the Sun.[13] The comet passed through the ecliptic of the Solar System at the end of October 2019, and made its closest approach to the Sun at just over 2 AU on 8 December 2019.[3][14] In November 2019, astronomers from Yale University said that the comet's tail was 14 times the size of Earth, and stated, "It's humbling to realize how small Earth is next to this visitor from another solar system."[15] In the middle of March, 2020, the comet was observed to fragment;[16] and later, in April, even more evidence of fragmentation was reported.[17][18][19]

Nomenclature

The comet is formally called "2I/Borisov" by the International Astronomical Union (IAU), with "2I" or "2I/2019 Q4" being its designation and "Borisov" being its name, but is sometimes referred to as "Comet Borisov", especially in the popular press.[c] As the second observed interstellar interloper after 1I/ʻOumuamua, it was given the "2I" designation, where "I" stands for interstellar.[20][8] The name Borisov follows the tradition of naming comets after their discoverers. Before final designation as 2I/Borisov, the object was referred to by other names:

  • Early orbit solutions suggested that the comet could be a near-Earth object and was thus listed on IAU's Minor Planet Center's (MPC) Near-Earth Object Confirmation Page (NEOCP) as gb00234.[21]
  • Further refinements after thirteen days of observation made clear the object was a hyperbolic comet, and it was given the designation C/2019 Q4 (Borisov) by the Minor Planet Center on 11 September 2019.[22] Astronomers such as Davide Farnocchia, Bill Gray, and David Tholen were already confident that the comet was interstellar.[22]
  • On 24 September 2019 the IAU announced that the Working Group for Small Body Nomenclature kept the name Borisov giving the comet the interstellar designation of 2I/Borisov, formally announcing the comet was indeed interstellar.[20][8]

Characteristics

In this observation, the NASA/ESA Hubble Space Telescope revisited the comet shortly after its closest approach to the Sun in December 2019.

Unlike ʻOumuamua, which had an asteroidal appearance, 2I/Borisov's nucleus is surrounded by a coma, a cloud of dust and gas.[23]

Comet 2I/Borisov and a distant galaxy (2MASX J10500165-0152029[24]) in November 2019.[25]

Size and shape

Early estimates of nucleus 2I/Borisov diameter have ranged from 1.4 to 16 km.[26][27] 2I/Borisov has, unlike Solar System comets, noticeably shrunk during Solar System flyby, losing at least 0.4% of its mass before perihelion.[7] Also, the amplitude of non-gravitational acceleration place an upper limit of 0.4 km on nucleus size, consistent with a previous Hubble Space Telescope upper limit of 0.5 km.[6] The comet did not come much closer to Earth than 300 million km, which prevents using radar to directly determine its size and shape. This could be done using the occultation of a star by 2I/Borisov but an occultation would be difficult to predict, requiring a precise determination of its orbit, and the detection would necessitate a network of small telescopes.[28]

Rotation

A study using observations from Hubble could not find a variation in the light curve. According to this study the rotational period must be larger than 10 hours.[29] A study with CSA's NEOSSat found a period of 13.2 ± 0.2 day, which is unlikely the nuclear spin.[30] Monte Carlo simulations based on the available orbit determinations suggest that the equatorial obliquity of 2I/Borisov could be about 59 degrees or 90 degrees, the latter is favored for the latest orbit determination.[31]

Chemical makeup and nucleus structure

Dave Jewitt and Jane Luu estimate from the size of its coma the comet is producing 2 kg/s of dust and is losing 60 kg/s of water. They extrapolate that it became active in June 2019 when it was between 4 and 5 AU from the Sun.[6] A search of image archives found precovery observations of 2I/Borisov as early as 13 December 2018, but not on 21 November 2018, indicating it became active between these dates.[32]

2I/Borisov's composition appears uncommon yet not unseen in Solar System comets, being relatively depleted in water and diatomic carbon (C2), but enriched in carbon monoxide and amines (R-NH2).[33] Molar ratio of carbon monoxide to water in 2I/Borisov tail is 35%-105%, resembling unusual blue-tailed comet C/2016 R2 while average for solar system comets is 4%.[34]

Trajectory

Trajectory across sky in cylindrical cooordinates, with 30 August 2019 discovery position along with precovery positions marked back to 13 December 2018 which help narrow down the incoming trajectory
Interstellar velocity inbound ()[d]
Object Velocity
1I/2017 U1 (ʻOumuamua) 26.33 km/s
5.55 AU/yr[35]
2I/2019 Q4 (Borisov) 32.2 km/s
6.79 AU/yr[36]

As seen from Earth, the comet was in the northern sky from September until mid-November. It crossed the ecliptic plane on 26 October near the star Regulus,[37] and the celestial equator on 13 November 2019, entering the southern sky. On 8 December 2019, the comet reached perihelion (closest approach to the Sun)[3] and near the inner edge of the asteroid belt.[e] In late December, it made its closest approach to Earth,[11][14] 1.9 AU, and had a solar elongation of about 80°.[5] Due to its 44° orbital inclination, 2I/Borisov does not make any notable close approaches to the planets.[3] 2I/Borisov entered the Solar System from the direction of Cassiopeia near the border with Perseus. This direction indicates that it originates from the galactic plane, rather than from the galactic halo.[36][38] It will leave the Solar System in the direction of Telescopium.[36][38] In interstellar space, 2I/Borisov takes roughly 9000 years to travel a light-year relative to the Sun.[f]

2I/Borisov's trajectory is extremely hyperbolic, having an orbital eccentricity of 3.36 .[3][4] This is much higher than the 300+ known weakly hyperbolic comets, with heliocentric eccentricities just over 1, and even ʻOumuamua with an eccentricity of 1.2 .[39][g] 2I/Borisov also has a hyperbolic excess velocity () of 32 km/s, much higher than what could be explained by perturbations, which could produce velocities when approaching an infinite distance from the Sun of less than a few km/s.[40] These two parameters are important indicators of 2I/Borisov's interstellar origin.[36][41] For comparison, the Voyager 1 spacecraft, which is leaving the Solar System, is traveling at 16.9 km/s (3.57 AU/a).[42] 2I/Borisov has a much larger eccentricity than ʻOumuamua due to its higher excess velocity and its significantly higher perihelion distance. At this larger distance, the Sun's gravity is less able to alter its path as it passes through the Solar System.[36]

2I/Borisov — orbit diagrams
Trajectory of Borisov (yellow) crossing the ecliptic plane; 'Oumuamua (red) shown for comparison
Borisov approaches the ecliptic plane between the orbits of Jupiter (pink) and Mars (orange)
Borisov's trajectory and position (white) as of 13 October 2019 (top view)

Observation

Discovery

The comet was discovered on 30 August 2019 by amateur astronomer Gennadiy Borisov at his personal observatory MARGO in Nauchnyy, Crimea, using a 0.65 meter telescope he designed and built himself.[43] The discovery has been compared to the discovery of Pluto by Clyde Tombaugh.[44] Tombaugh was also an amateur astronomer who was building his own telescopes, although he discovered Pluto using Lowell Observatory's astrograph. At discovery, it was inbound 3 AU from the Sun, 3.7 AU from Earth, and had a solar elongation of 38°.[45] Borisov described his discovery thus:[46]

JPL Scout eccentricity ranges[47]
# of
observations 		Observation
arc (hours) 		Eccentricity
range
81 225 0.9–1.6
99 272 2.0–4.2
127 289 2.8–4.7
142 298 2.8–4.5
151 302 2.9–4.5

I observed it on August 29, but it was August 30 Greenwich Time.[h] I saw a moving object in the frame, it moved in a direction that was slightly different from that of main asteroids.[i] I measured its coordinates and consulted the Minor Planet Center database. Turned out, it was a new object. Then I measured the near-Earth object rating,[j] it is calculated from various parameters, and it turned out to be 100% – in other words, dangerous. In such cases I must immediately post the parameters to the world webpage for confirmation of dangerous asteroids.[k] I posted it and wrote that the object was diffuse and that it was not an asteroid, but a comet.

2I/Borisov's interstellar origin required a couple of weeks to confirm. Early orbital solutions based on initial observations included the possibility that the comet could be a near-Earth object 1.4 AU from the Sun in an elliptical orbit with an orbital period of less than 1 year.[21] Later using 151 observations over 12 days, NASA Jet Propulsion Laboratory's Scout gave an eccentricity range of 2.9–4.5 .[48] But with an observation arc of only 12 days, there was still some doubt that it was interstellar because the observations were at a low solar elongation, which could introduce biases in the data such as differential refraction. Using large non-gravitational forces on the highly eccentric orbit, a solution could be generated with an eccentricity of about 1, an Earth minimum orbit intersection distance (MOID) of 0.34 AU (51 million km), and a perihelion at 0.90 AU around 30 December 2019.[49] However, based on available observations, the orbit could only be parabolic if non-gravitational forces (thrust due to outgassing) affected its orbit more than any previous comets.[50] Eventually with more observations the orbit converged to the hyperbolic solution that indicated an interstellar origin and non-gravitational forces could not explain the motion.[22]

Observation tools

Hubble started observations of 2I/Borisov in October 2019, two months prior to the comet's closest approach to the Sun

Unless the comet fades or disintegrates unexpectedly, it should be observable until at least September 2020[needs update].[22] Observation of 2I/Borisov is aided by the fact that the comet was detected while inbound towards the Solar System. ʻOumuamua had been discovered as it was leaving the system, and thus could only be observed for 80 days before it was out of range. Because of its closest approach occurring near traditional year-end holidays, and the capability to have extended observations, some astronomers have called 2I/Borisov a "Christmas comet".[13][51] Observations using the Hubble Space Telescope began on 12 October, when the comet moved far enough from the Sun to be safely observed by the telescope.[52] Hubble is less affected by the confounding effects of the coma than ground-based telescopes, which will allow it to study the rotational light curve of 2I/Borisov's nucleus. This should facilitate an estimate of its size and shape. The observations will serve as a baseline for possible further observations, as the comet approaches perihelion and then leaves the Solar System.

Comet chemistry

A preliminary (low-resolution) visible spectrum of 2I/Borisov was similar to typical Oort Cloud comets.[53][54] Its color indexes also resemble the Solar System's long period comets.[6] Emissions at 388 nm indicated the presence of cyanide (formula CN), which is typically the first detected in Solar System comets including comet Halley.[55] This was the first detection of gas emissions from an interstellar object.[56] The non-detection of diatomic carbon has also been reported in October 2019, with the ratio C2 to CN being less than either 0.095[57] or 0.3 .[58] The diatomic carbon was positively detected in November 2019, with measured C2 to CN ratio of 0.2±0.1 .[59] This resembles a carbon-chain depleted group of comets. These are either Jupiter family comets,[57] or rare blue-colored carbon monoxide comets exemplified by C/2016 R2 comet.[60] By the end of November 2019, C2 production have dramatically increased, and C2 to CN ratio have reached 0.61, along with appearance of bright amine (NH2) bands.[61] Atomic oxygen has also been detected, from this observers estimated an outgassing of water at a rate similar to Solar System comets.[62][63] Initially, neither water nor OH lines were directly detected[64] in September 2019. First unambiguous detection of OH lines was done 1 November 2019, and OH production peaked in early December 2019.[65]

Suspected nucleus fragmentation

The comet did come within about 2 AU of the Sun, a distance at which many small comets have been found to disintegrate. The probability that a comet disintegrates strongly depends on the size of its nucleus; Guzik et al. estimated a probability of 10% that this will happen to 2I/Borisov.[66] Jewitt and Luu compared 2I/Borisov to C/2019 J2, another comet of similar size that disintegrated in May 2019 at a distance of 1.9 AU from the Sun.[67][6] In the event that the nucleus disintegrates, as is sometimes seen with small comets, Hubble can be used to study the evolution of the disintegration process.[68][6]

The severe outburst in February-March 2020, led to suspected "ongoing nucleus fragmentation" from the comet by March 12.[16] Indeed, images from the Hubble Space Telescope taken on 30 March 2020 show a non-stellar core indicating that Comet 2I/Borisov has ejected sunward a large fragment.[17][18][69] The ejection is estimated to have begun around 7 March,[70] and may have occurred during one of the outbursts that occurred near that time.[71] The ejected fragment appeared to have vanished by 6 April 2020.[72]

A followup study, reported on 6 April 2020, observed only a single object, and noted that the fragment component had now disappeared.[72][19] Later analysis of the event showed the ejected dust and fragments have a combined mass of about 0.1% of total mass of nucleus, making event a large outburst rather than fragmentation.[73]

Exploration

The higher hyperbolic excess velocity of 2I/Borisov of 32 km/s makes it even harder to reach for a spacecraft than 1I/'Oumuamua (26 km/s).[dubious – discuss] According to a team of the Initiative for Interstellar Studies, a two-ton spacecraft could theoretically have been sent in July 2018 to intercept 2I/Borisov using a Falcon Heavy-class launcher, but only if the object had been discovered much earlier than it was. Launches after the actual discovery date would require a significantly larger launcher such as the Space Launch System (SLS) and Oberth manoeuvres near Jupiter and near the Sun. By September 2019, even an SLS-class launcher would only be able to deliver a 3 kg (6.6 lb) payload (such as a CubeSat) into a trajectory that could intercept 2I/Borisov in 2045 at a relative speed of 34 km/s.[74] According to congressional testimony, NASA may need at least five years of preparation to launch such an intercepting mission.[75]

See also

Notes

  1. ^ A photograph of Borisov's dust trail taken on 12 October 2019 with the UVIS F350LP channel of Wide Field Camera 3 aboard the Hubble Space Telescope.[1][2] At the time of this photograph, Borisov was 418,000,000 kilometres (260,000,000 mi) from Earth, similar to the average distance of the asteroid Ceres from the Sun, and traveling at a velocity of 177,000 kilometres per hour (110,000 mph).[2]
  2. ^ Objects with eccentricities greater than 1 will have a negative semimajor axis, giving them a positive orbital energy – the smaller the perihelion distance, and the larger above 1 the eccentricity is, the closer to 0 the semimajor axis value will be.
  3. ^ This is the eighth comet discovered by Gennadiy Borisov, and thus the ambiguous term "Comet Borisov" is not formally used here.
  4. ^ For objects gravitationally bound to the Sun, velocities when approaching the equivalent of an infinite distance from the Sun should be less than a few kilometres per second. At its furthest distance from the Sun, Halley's comet moves ≈ 1 km/s with respect to the Sun.
  5. ^ 2I/Borisov will come to perihelion outside the orbit of Mars at a distance of 2.01 AU, which is just inside the 4:1 Kirkwood gap located at 2.06 AU.
  6. ^ 299792.458 km/s / 32.2 km/s = 9310 times slower than light.
  7. ^ A comet with a parabolic trajectory (with an eccentricity of 1) would leave the Solar System in the direction it entered, having had its path altered by 180°. 2I/Borisov, with its higher eccentricity, has a more open trajectory and will have its path altered by only 34° as it passes through the Solar System.
  8. ^ This is obviously a mistake: Crimea is 3 hours ahead of Greenwich, so it was August 30 in Crimea when Borisov first observed the comet.
  9. ^ Of the 850,000 objects known to orbit the Sun, 756,000 (89%) are main-belt asteroids.
  10. ^ NEO Rating for calculating the probability that a new object is a near-Earth candidate.
  11. ^ The NEO Confirmation Page for confirming near-Earth objects and potentially hazardous objects.

References

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  2. ^ a b National Aeronautics and Space Administration; European Space Agency; Jewitt, David (16 October 2019). "Hubble observes cirst confirmed interstellar comet". Hubblesite. Archived from the original on 17 October 2019. Retrieved 17 October 2019. Hubble took a series of snapshots as the comet streaked along at 110,000 miles per hour. [...] The comet was 260 million miles from Earth when Hubble took the photo. [...] This Hubble image, taken on 12 October 2019 [...] reveals a central concentration of dust around the nucleus (which is too small to be seen by Hubble).
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    "99 obs / 272 hours". JPL CNEOS. Scout: gb00234. Archived from the original on 10 September 2019.
    "127 obs / 289 hours". JPL CNEOS. Scout: gb00234. Archived from the original on 11 September 2019.
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