2I/Borisov

From Wikipedia, the free encyclopedia
  (Redirected from C/2019 Q4 (Borisov))
Jump to navigation Jump to search
2I/Borisov
Borisov Hubble first image.png
Hubble Space Telescope image of 2I/Borisov taken on 12 October 2019 using the Wide Field Camera 3.[1][2]
Discovery
Discovered byGennadiy Borisov at MARGO observatory, Nauchnyy, Crimea
Discovery date30 August 2019
Alternative
designations
  • 2I
  • 2I/2019 Q4
  • 2I/Borisov
  • 2I/2019 Q4 (Borisov)
  • C/2019 Q4 (Borisov)
  • gb00234
Orbital characteristics A
Epoch17 September 2019[3]
Observation arc40 days
Number of
observations
424
Perihelion2.006±0.001 au
Semi-major axis−0.852±0.001 au[Note 1]
Eccentricity3.354±0.005 (JPL)
3.355 (MPC)[4]
3.335±0.005 (Gray)[5]
Inclination44.06°±0.01°
Node308.14°±0.01°
Peri209.14°±0.02°
Earth MOID1.09 au
Jupiter MOID2.39 au
Dimensions2 km[2][6][7]
1.4–6.6 km[8]
450–550 m[9] (for an albedo of 0.04)
2–16 km[10]
Next perihelion8 December 2019[3][4][5]

2I/Borisov, originally designated C/2019 Q4 (Borisov),[7][11] is the first observed interstellar comet[1][2] and the second observed interstellar interloper after ʻOumuamua.[12][13] 2I/Borisov has a heliocentric orbital eccentricity of 3.3 and is not bound to the Sun.[3] The comet will pass through the ecliptic of the Solar System in December 2019, with the closest approach to the Sun at just under au on 8 December 2019.

Nomenclature[edit]

The comet is formally named "2I/Borisov" by the International Astronomical Union (IAU), but is sometimes referred to as "Comet Borisov", especially in the popular press.[Note 2] As the second observed interstellar interloper after 1I/ʻOumuamua, it was given the "2I" designation, where "I" stands for interstellar.[7][11] 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.[14]
  • 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.[15] Astronomers such as Davide Farnocchia, Bill Gray, and David Tholen were already confident that the comet was interstellar.[15]
  • 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.[7][11]

Characteristics[edit]

Physical characteristics[edit]

Unlike ʻOumuamua, which had an asteroidal appearance, Borisov's initial observations and subsequent third-party validation affirmed the presence of a coma around the body, indicating a cloud of dust and gas that would classify the body as a comet.[16] 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.[17] Initial estimates for the size of 2I/Borisov's nucleus, published on 12 September 2019, ranged from 2 to 16 km, based on observations made by Karen Meech at the University of Hawaii,[10] while Guzik et al. estimated a size of about 0.5 km, assuming an albedo of 0.04.[9] On 18 September, Siraj et al. argued that the nucleus was likely small, on the order of 2 km.[6] An improved size estimate, based on the production rate of certain molecules in the comet's coma, was published by Alan Fitzsimmons, Karen Meech and others on 26 September. They estimated that the nucleus is between 1.4 and 6.6 km in diameter.[8]

On 13 September 2019, the Gran Telescopio Canarias obtained a preliminary (low-resolution) visible spectrum of 2I/Borisov that revealed that this comet has a composition not very different from that found in typical Oort Cloud comets.[18][19] Similarly, measurements taken at the Nordic Optical Telescope found the comet had color indexes resembling the Solar System's long period comets.[17] The William Herschel Telescope, located at the island of La Palma, reported the detection of cyanide (formula CN) emission at 388 nm (this type of emission has been detected in many other comets, including comet Halley)[20] and put constraints on the production rate of other molecules such as diatomic carbon (formula C2).[8] This was the first detection of gas emissions from an interstellar object.[20] Later observation at the Bok telescope and MMT telescope in Arizona detected diatomic carbon. The ratio of C2 to CN is similar to a depleted group of comets, most of which are Jupiter family comets.[21]

The comet will 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.[9] 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.[17][22] If 2I/Borisov disintegrates, it is possible that it leaves behind an inactive remnant, similar to 'Oumuamua.[17][23]

Trajectory[edit]

Interstellar velocity inbound ()[Note 3]
Object Velocity
1I/2017 U1 (ʻOumuamua) 26.33 km/s
5.55 au/yr[24]
2I/2019 Q4 (Borisov) 32.2 km/s
6.79 au/yr[25]

As seen from Earth, the comet is in the northern sky from September until mid-November. It will cross the ecliptic plane on 13 November 2019 entering the southern sky. On 6 December 2019, the comet will be an equal distance of 2 au from the Sun and Earth.[5] On 8 December 2019, the comet will come to perihelion (closest approach to the Sun)[3] and will be near the edge of the inner asteroid belt.[Note 4] In late December, it will be about 1.9 au from Earth and have 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.[25] In interstellar space, 2I/Borisov takes roughly 9000 years to travel a light-year relative to the Sun.[Note 5] It will leave the Solar System in the direction of Telescopium.[25] 2I/Borisov has passed within 5.7 light-years of the binary star system Kruger 60 (13.18 light-years away, in Cepheus) at a low velocity of 3.4 km/s around a million years ago.[26]

2I/Borisov's trajectory is extremely hyperbolic, having an orbital eccentricity of 3.3 to 3.4.[3][4][5] 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.[27][Note 6] 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.[28] These two parameters are important indicators of 2I/Borisov's interstellar origin.[25][29] For comparison, the Voyager 1 spacecraft, which is leaving the Solar System, is traveling at 16.9 km/s (3.57 au/yr).[30] 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.[25]

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

Observation[edit]

Discovery[edit]

JPL Scout eccentricity ranges[31]
# 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

The comet was discovered on 30 August 2019 by amateur astronomer Gennadiy Borisov at his personal observatory MARGO using a 0.65-meter telescope he designed and built himself.[32] The discovery has been compared to the discovery of Pluto by Clyde Tombaugh.[33] 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°.[34] Borisov described his discovery thus:[35]

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.[14] Later using 151 observations over 12 days, NASA Jet Propulsion Laboratory's Scout gave an eccentricity range of 2.9–4.5.[36] 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.[37] 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.[38] 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.[15] 2I/Borisov's trajectory was better resolved with a larger observation arc collected from additional observatories. After a 13-day observation arc, a best-fit for the hyperbolic orbit had an eccentricity of about 3.5, with perihelion at 2 au.[5]

Planned observations[edit]

Unless the comet fades or disintegrates unexpectedly, it should be observable until at least September 2020.[15] 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".[39] Observations using the Hubble Space Telescope began on October 12, when the comet moved far enough from the Sun to be safely observed by the telescope.[40] 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. 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.[41][17]

Exploration[edit]

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 ] 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.[42] According to congressional testimony, NASA may need at least five years of preparation to launch such an intercepting mission.[43]

See also[edit]

Notes[edit]

  1. ^ 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.
  2. ^ This is the eighth comet discovered by Gennadiy Borisov, and thus the ambiguous term "Comet Borisov" is not formally used here.
  3. ^ 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.
  4. ^ 2I/Borisov will come to perihelion outside the orbit of Mars at a distance of 1.99 au, which is just inside of the 4:1 Kirkwood gap located at 2.06 au.
  5. ^ 299792.458 km/s / 32.2 km/s = 9310 times slower than light.
  6. ^ 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.
  7. ^ 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.
  8. ^ Of the 800,000 objects known to orbit the Sun, 737,000 (92%) are main-belt asteroids.
  9. ^ NEO Rating for calculating the probability that a new object is a near-Earth candidate.
  10. ^ The NEO Confirmation Page for confirming near-Earth objects and potentially hazardous objects.

References[edit]

  1. ^ a b Astronomical Observatory, Jagiellonian University (14 October 2019). "Interstellar Comet with a Familiar Look". EurekAlert!. Retrieved 14 October 2014.
  2. ^ a b c Guzik, Piotr; et al. (14 October 2019). "Initial characterization of interstellar comet". Nature Astronomy. 136. doi:10.1038/s41550-019-0931-8. Retrieved 14 October 2019.
  3. ^ a b c d e f "JPL Small-Body Database Browser: C/2019 Q4 (Borisov)". Jet Propulsion Laboratory. Archived from the original on 2019-10-03. Retrieved 2019-10-03.
  4. ^ a b c "2I/Borisov=C/2019 Q4 (Borisov)". Minor Planet Center. 2019-10-01. Retrieved 2019-10-05.
  5. ^ a b c d e f Gray, Bill (2019-09-20). "Pseudo-MPEC for gb00234". Project Pluto. Archived from the original on 2019-09-11. Retrieved 2019-09-20.
  6. ^ a b Siraj, Amir; Loeb, Abraham (2019). "An Argument for a Kilometer-Scale Nucleus of C/2019 Q4". Research Notes of the American Astronomical Society. 3 (9): 132. arXiv:1909.07286. Bibcode:2019RNAAS...3..132S. doi:10.3847/2515-5172/ab44c5.
  7. ^ a b c d Christensen, Lars Lindberg. "Naming of New Interstellar Visitor: 2I/Borisov" (Press release). International Astronomical Union. Retrieved 24 September 2019.
  8. ^ a b c Fitzsimmons, Alan; Hainaut, Olivier; Meech, Karen; Jehin, Emmanuel; Moulane, Youssef; Opitom, Cyrielle; Yang, Bin; Keane, Jacqueline V.; Kleyna, Jan T.; Micheli, Marco; Snodgrass, Colin (2019). "Detection of CN gas in Interstellar Object 2I/Borisov". arXiv:1909.12144 [astro-ph.EP].
  9. ^ a b c Guzik, Piotr; Drahus, Michał; Rusek, Krzysztof; Waniak, Wacław; Cannizzaro, Giacomo; Pastor-Marazuela, Inés (2019). "Interstellar comet 2I/Borisov". arXiv:1909.05851v1 [astro-ph.EP].
  10. ^ a b Newly Discovered Comet Is Likely Interstellar Visitor NASA, September 12, 2019
  11. ^ a b c "MPEC 2019-S72 : 2I/Borisov=C/2019 Q4 (Borisov)". Minor Planet Center. Retrieved 24 September 2019.
  12. ^ Grossman, Lisa (2019-09-12). "Astronomers have spotted a second interstellar object". Science News. Retrieved 2019-09-16.
  13. ^ Strickland, Ashley (24 September 2019). "2nd interstellar visitor to our solar system confirmed and named". CNN.
  14. ^ a b Gray, Bill. "Pseudo-MPEC for gb00234 (AutoNEOCP)". Project Pluto. Archived from the original on 2019-09-10. Retrieved 2019-09-13.
  15. ^ a b c d "COMET C/2019 Q4 (Borisov)". Minor Planet Center. Retrieved 2019-09-11.
  16. ^ Greskno, Michael (12 September 2019). "Bizarre comet from another star system just spotted". National Geographic. Retrieved 25 September 2019.
  17. ^ a b c d e Jewitt, David; Luu, Jane (2019). "Initial Characterization of Interstellar Comet 2I/2019 Q4 (Borisov)". arXiv:1910.02547 [astro-ph.EP].
  18. ^ "The Gran Telescopio Canarias (GTC) obtains the visible spectrum of C/2019 Q4 (Borisov), the first confirmed interstellar comet". Instituto Astrofisico de Canarias. Retrieved 2019-09-14.
  19. ^ de León, Julia; Licandro, Javier; Serra-Ricart, Miquel; Cabrera-Lavers, Antonio; Font Serra, Joan; Scarpa, Riccardo; de la Fuente Marcos, Carlos; de la Fuente Marcos, Raúl (19 September 2019). "Interstellar Visitors: A Physical Characterization of Comet C/2019 Q4 (Borisov) with OSIRIS at the 10.4 m GTC". Research Notes of the American Astronomical Society. 3 (9): 131. Bibcode:2019RNAAS...3..131D. doi:10.3847/2515-5172/ab449c.
  20. ^ a b "IAU Electronic Telegram No. 4670". Central Bureau for Astronomical Telegrams. Retrieved 2019-09-25.
  21. ^ Kareta, Theodore; Andrews, Jennifer; Noonan, John W.; Harris, Walter M.; Smith, Nathan; O'Brien, Patrick; Sharkey, Benjamin N. L.; Reddy, Vishnu; Springmann, Alessondra; Lejoly, Cassandra. "Carbon Chain Depletion of 2I/Borisov". arXiv:1910.03222.
  22. ^ Jewitt, David; Luu, Jane (2019). "Disintegrating Inbound Long-period Comet C/2019 J2". The Astrophysical Journal Letters. 883 (2). arXiv:1909.01964. doi:10.3847/2041-8213/ab4135.
  23. ^ Sekanina, Zdenek (2019). "1I/`Oumuamua and the Problem of Survival of Oort Cloud Comets Near the Sun". arXiv:1903.06300 [astro-ph.EP].
  24. ^ Gray, Bill (26 October 2017). "Pseudo-MPEC for A/2017 U1 (FAQ File)". Project Pluto. Retrieved 26 October 2017.
  25. ^ a b c d e Gray, Bill. "FAQ for C/2019 Q4 (Borisov)". Project Pluto. Retrieved 2019-09-25.
  26. ^ Dybczyński, Piotr A.; Królikowska, Małgorzata; Wysoczańska, Rita (2019). "Kruger 60 -- a plausible home system of the interstellar comet C/2019 Q4". arXiv:1909.10952 [astro-ph.EP].
  27. ^ "JPL Small-Body Database Search Engine: e > 1". Jet Propulsion Laboratory. Archived from the original on 2019-09-25. Retrieved 2019-09-25.
  28. ^ Siegel, Ethan (2017-12-16). "Ask Ethan: Why Don't Comets Orbit The Same Way Planets Do?". Archived from the original on 2019-10-01. Retrieved 2019-10-01.
  29. ^ "Interstellar Comet gb00234". Astronomer's Telegram. Archived from the original on 2019-09-12. Retrieved 2019-09-12.
  30. ^ "Fast Facts". Jet Propulsion Laboratory – Voyager. Retrieved 27 September 2019.
  31. ^ Scout: gb00234 at Archive.is: (81 obs / 225 hours) (99 obs / 272 hours) (127 obs / 289 hours) (142 obs / 298 hours) (151 obs / 302 hours)
  32. ^ King, Bob (11 September 2019). "Is Another Interstellar Visitor Headed Our Way?". Sky & Telescope. Retrieved 12 September 2019.
  33. ^ Нелюбин, Николай (13 September 2019). «Готовы открывать кометы бесплатно, лишь бы имя осталось». Российский астроном Геннадий Борисов о первой в истории человечества межзвёздной комете [“We’ll discover comets without pay, what matters is that the name lives on”. Russian astronomer Gennadiy Borisov on the first interstellar comet in the history of humankind]. Fontanka.ru [ru] Фонтанка.ру (in Russian). Retrieved September 16, 2019.
  34. ^ Gray, Bill. "Pseudo-MPEC for gb00234 (precovery-eph)". Project Pluto. Archived from the original on 2019-09-12. Retrieved 2019-09-11.
  35. ^ Крымский астроном заявил, что открытая им комета изменит название [Crimean astronomer says that the comet discovered by him will be renamed]. RIA Novosti РИА Новости (in Russian). 16 September 2019. para. 5. Retrieved 16 September 2019.
  36. ^ "Scout: gb00234". JPL CNEOS. Archived from the original on 2019-09-10. Retrieved 2019-09-10. (archive.is with 151 obs)
  37. ^ Gray, Bill (2019-09-10). "Is gb00234 an Interstellar Comet or Asteroid". Minor Planet Mailing List. Retrieved 2019-09-10.
  38. ^ Gray, Bill. "Pseudo-MPEC for gb00234 (non-grav A1+A2)". Project Pluto. Archived from the original on 2019-09-11. Retrieved 2019-09-11.
  39. ^ Overbye, Dennis (1 October 2019). "An Interstellar Comet, in Time for the Holidays - On Dec. 7, the extrasolar comet now known as 2I/Borisov will make its closest approach to the sun". The New York Times. Retrieved 2 October 2019.
  40. ^ HST Weekly Observing Timeline, Space Telescope Science Institute, 7 October 2019, retrieved 8 October 2019
  41. ^ Jewitt, D.; Weaver, H. A.; Mutchler, M.; Agarwal, J.; Kim, Y.; Hui, M.-T. (25 September 2019). "Proposal 16009 - Interstellar Object C/2019 Q4" (PDF). Space Telescope Science Institute. Retrieved 27 September 2019.
  42. ^ Hibberd, Adam; Perakis, Nikolaos; Hein, Andreas M. (2019). "Sending a Spacecraft to Interstellar Comet C/2019 Q4 (Borisov)". arXiv:1909.06348 [astro-ph.EP].
  43. ^ U.S. Congress (19 March 2013). "Threats From Space: A Review of U.S. Government Efforts to Track and mitigate Asteroids and Meteors (Part I and Part II) – Hearing Before the Committee on Science, Space, and Technology House of Representatives One Hundred Thirteenth Congress First Session" (PDF). p. 147. Retrieved 14 September 2019.

External links[edit]