AI 2023. Meet ChatGPT. - page 74

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The next scheduled tests are:

5 and 6: comparing the quality of human and ChatGPT structuring of subject information.


Disciplines selected for testing:

  • Astronomy
  • Physics
  • Zoology
 

Astronomy:

Solar System:

CHATGP:

Promt: Tell us all about the Solar System.

...

The Solar System is a system of planets, comets, asteroids, and other space objects that revolve around the Sun. The Sun is the central body of the Solar System and has almost 99% of the mass of the entire system.

Here are some facts about the Solar System:

  1. There are eight planets in the Solar System that move around the Sun. They are called Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus, and Neptune.

  2. Pluto used to be considered the ninth planet in the Solar System, but was reclassified as a dwarf planet in 2006.

  3. Each planet has its own orbit around the Sun. For example, Mercury moves faster than any other planet and orbits the Sun completely in 88 Earth days, while Neptune orbits the Sun completely in 165 Earth years.

  4. In addition to planets, there are also asteroids, comets, space dust and gas in the Solar System. Comets, for example, are icy bodies that pass through the interior of the Solar System and can collide with planets.

  5. The Solar System was formed about 4.6 billion years ago. Scientists believe it formed from a huge cloud of gas and dust that began to collapse under the force of gravity.

  6. The Sun is a star that sits at the centre of the Solar System. It is the main source of energy and heat for all the planets and other objects in the system.

  7. The Solar System is located in the Milky Way galaxy, and occupies part of the spiral of this galaxy.

  8. Exploration of the Solar System is one of the major areas of space exploration. NASA and other space agencies send probes and spacecraft to study the Solar System and its objects in more detail. For example, the Voyager probe flew past all of the outer planets of the Solar System in the 1970s, and the New Horizons probe passed Pluto in 2015.

  1. Studying the Solar System gives us a better understanding of how our universe works and how life can arise and evolve elsewhere in the cosmos.

  2. The Solar System is in constant motion, and it may collide with another star system or other space objects in the future. Such collisions could have serious consequences, but the probability of their occurrence is low.

Overall, the Solar System is an amazing and complex cosmic object that continues to interest and fascinate scientists and space enthusiasts.

...


Wikipedia: Solar system - Wikipedia (wikipedia.org )

 

Solar system

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Material from Wikipedia, the free encyclopaedia
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Solar system
Solar System size to scale ru.svg
The solar system as imagined by the artist. The scale of distances from the Sun is not respected
General characteristics
Age 4.5682±0.0006billion years [1][2]
Location Local interstellar cloud,Local bubble,Orion arm,Milky Way,Local group of galaxies
Mass 1,0014 M☉
Nearest star Proxima Centauri ( 4.21-4.24sv years)[3]
Alpha Centauri System ( 4.37 sv years)[4]
Third space velocity(near theEarth's surface) 16.65 km/s
Planetary system
The most distant planet from the Sun Neptune(4.503 billion kilometres,30.1a.u.)[5]
Distance to theKuiper belt ~30-50 a.u.[6]
Number ofstars 1(Sun)
Number of known planets 8
Number ofdwarf plan ets 5[7]
Number ofsatellites 639 (204 for planets and 435 forsmall solar systembodies)[8][9]
Number of small bodies More than1,000,000 ( as of November 2020)[8]
Number ofcomets 3,690 (as of November 2020)[8]
Circumference around the galactic centre
Inclination to the plane of the Milky Way 60,19°
Distance to thegalactic centre 27 170±1140 sv years
(8330±350pc)[10]
Circulation period 225-250 million years [11]
Orbital velocity 220-240 km/s[12]
Properties associated with the star
Spectral class G2 V[13][14]
Snow line ~5 a.u.[15][16]
Heliospheric boundary ~113-120 a.u.[17]
Radius ofHill's sphere ~1-2 sv. years

Planetary System.
(Geographical Atlas for Gymnasiums, 1898 ).

Thesolar system is a planetary system that includes the centralstar the Sun and all naturalspace objects in heliocentric orbits. It was formed bygravitational compression of agas-dust cloud about 4.57 billion years ago[2].

The total mass of the solar system is about 1.0014M☉ . Most of it is in the Sun; the remaining part is almost entirely contained in eight distantplanets with nearly circularorbits lying almost in the same plane, theecliptic plane. Because of this, a contradictory distribution ofmomentum between the Sun and the planets (the so-called "momentum problem") is observed: only 2 % of the total momentum of the system falls on the Sun, whose mass is ~740 times greater than the total mass of the planets, and the remaining 98 % - on ~0.001 of the total mass of the solar system[18].

The four planets closest to the Sun, called theterrestrial group planets,Mercury,Venus,Earth[19] and Mars, are composed primarily ofsilicates and metals. The four planets more distant from the Sun, calledgiant plan ets - Jupiter,Saturn,Uranus, and Neptune - are much more massive than the Earth-group planets. The largest giant planets in the solar system, Jupiter and Saturn, are composed primarily ofhydrogen and helium and are therefore classified asgas giants; the smaller giant planets - Uranus and Neptune - in addition to hydrogen and helium, predominantly containwater,methane and ammonia; such planets are classified as a separate class of "ice g iants"[20]. Six of the eight planets and fourdwarf planets have naturalsatellites. Jupiter, Saturn, Uranus, and Neptune are surrounded byrings of dust and other particles.

There are two regions in the solar system filled withsmall bodies. Theasteroid belt, located between Mars and Jupiter, is similar in composition to the Earth-group planets in that it is made up of silicates and metals. The largest objects in the asteroid belt are the dwarf planetCeres and the asteroidsPallada,Vesta and Hygeia. Beyond the orbit of Neptune aretrans-Neptunian objects composed offrozen water , ammonia and methane, the largest of which arePluto,Sedna,Haumea,Makemake,Kvavar,Ork and Erida. Other populations of small bodies exist in the solar system, such as planetaryquasi-satellites and Trojans,near-Earth asteroids,centaurs,damocloids, andcomets,meteoroids, and cosmic dust travelling through the system.

Thesolar wind (the flow ofplasma from the Sun) creates abubble in the interstellar medium called theheliosphere, which extends to the edge of thescattered disc. The hypotheticalOort cloud, which serves as the source of long-period comets, may extend about a thousand times further than the heliosphere.

 
This is the tenth part of Wikipedia's description of the Solar System. There are countless references, tables, illustrations, diagrams, interactive content, links to sources, and more...
 
Реter Konow #:

Astronomy:

Solar System:

***

Ask if there is a pattern in the distance of planets from the sun. And what are the odds that the asteroid belt was a planet

 
There's no point in comparing them. It's like comparing an adult to a newborn. Just see the difference.
 
Vitaliy Kuznetsov #:

Ask if there is a pattern in the distance of planets from the sun. And what are the odds that the asteroid belt was a planet

Now we do the basic testing and then move on to the rest of the questions.

 

Notes[edit | edit code]

  1. ↑Bowring S., Housh T. The Earth's early evolution // Science. - 1995. - Vol .269,no.5230. - P.1535-1540. - doi:10.1126/science.7667634. - Bibcode: 1995Sci...269.1535B. - PMID 7667634.
  2. ↑Jump back:12Bouvier, Audrey and Meenakshi Wadhwa.The age of the Solar System redefined by the oldest Pb-Pb age of a meteoritic inclusionArchived 11 October 2011 at theWayback Machine.Nature Geoscience, Nature Publishing Group, a division of Macmillan Publishers Limited. Published online 2010-08-22, retrieved 2010-08-26,doi:10.1038/NGEO941
  3. ↑Cosmic Distance Scales - The Nearest Star.Date of access: 2 December 2012.Archived from theoriginal on 18 January 2012.
  4. ↑Planet Found in Nearest Star System to Earth.European Southern Observatory ( 16 October 2012). Date accessed: 17 October 2012.Archived 23 November 2012.
  5. ↑Jump back:12Podolak, M.; Reynolds, R. T.; Young, R.Post Voyager comparisons of the interiors of Uranus and Neptune . NASA Ames Research Center (1990).Date of access: 22 November 2009.Archived 22 August 2011.
  6. ↑Alan Stern; Colwell, Joshua E.Collisional Erosion in the Primordial Edgeworth-Kuiper Belt and the Generation of the 30-50 AU Kuiper Gap //The Astrophysical Journal: journal . - IOP Publishing, 1997. - Vol.490,no.2. - P.879-882. doi:10.1086/304912.Archived 14 July 2014.
  7. ↑Mike Brown.Free thedwarf planets!Mike Brown's Planets (self-published) ( 23 August 2011).Date access ed: 24 December 2012.Archived 25 December 2012.
  8. ↑Jump back:123How Many Solar System Bodies. NASA/JPL Solar System Dynamics.Date accessed: 9 November 2012.Archived 5 December 2012.
  9. ↑Wm.Robert Johnston.Asteroids with Satellites. Johnston's Archive (28 October 2012).Date accessed: 9 November 2012.Archived 4 December 2012.
  10. ↑Gillessen, S.; Eisenhauer; Trippe; Alexander; Genzel; Martins; Ott. Monitoring Stellar Orbits Around the Massive Black Hole in the Galactic Centre //The Astrophysical Journal: journal. - IOP Publishing, 2009. - Vol .692,no.2. - P.1075-1109. - doi:10.1088/0004-637X/692/2/1075. - Bibcode: 2009ApJ...692.1075G. - arXiv:0810.4674.
  11. ↑Jump back:123Stacy Leong.Period of theSun's Orbit around the Galaxy (Cosmic Year ).The Physics Factbook ( 2002 ).Date of access:28 December 2009.Archived 22 August 2011.
  12. ↑Life on Earth is threatened by "galactic dives".Grani.ru.Date of access: 24 December 2012.Archived 25 February 2013.
  13. ↑ESO - Astronomical Glossary. Date of access: 8 September 2013.Archived 1 February 2014.
  14. ↑The Solar System. Date of access: 20 January 2014.Archived 30 May 2013.
  15. ↑M.J. Mumma, M. A. DiSanti, N. Dello Russo, K. Magee-Sauer, E. Gibb, R. Novak. Remote infrared observations of parent volatiles in comets: A window on the early solar system .) //Advances in Space Research ( English ) Russian: journal. - Elsevier, 2003. - Vol.31,no.12. - P.2563-2575. doi:10.1016/S0273-1177(03)00578-7.
  16. ↑Kaufmann, William J.Discovering the Universe - W.H. Freeman and Company (English) Russian, 1987. - P. 94. - ISBN 0-7167-1784-0.
  17. ↑NASA's Voyager Hits New Region at Solar System Edge 12.05.11.Date of access: 24 December 2012.Archived 8 March 2015.
  18. ↑Andreev V. D. Distribution of Moments in the Solar Planetary System // Newest Problems of Field Theory 2005-2006 (ed. by A. V. Aminova), Izd. of Kazan, Kazan, 2007, pp. 42-56. //also inAndreev,V. D. Selected problems of theoretical physics.D.Selected Problems of Theoretical Physics- Kiev: Avanpost-Prim, 2012.Archived 4 September 2017 at theWayback Machine
  19. ↑Velichko K. I.,Vitkovsky V.V. V.,Polenov B. K.,Sobichevsky V.T.Earth // TheEncyclopaedic Dictionary of Brockhaus and Efron: in 86 vols. (82 vol. and 4 supplements). - St. Petersburg. , 1890-1907.
  20. ↑There must be a powerful layer of superionic water in the structure of ice giants. Compulenta (3 September 2010).Date of access: 9 October 2011.Archived from theoriginal on 5 September 2010.
  21. ↑M.Woolfson . The origin and evolution of the solar system // Astronomy & Geophysics. - 2000. - Vol.41. - P.1.12. - doi:10.1046/j.1468-4004.2000.00012.x.
  22. ↑Harold F. Levison, Alessandro Morbidelli,The formation of the Kuiper belt by the outward transport of bodies during Neptune's migration (PDF ) ( 2003).Date of access: 23 November 2009.Archived 22 August 2011.
  23. ↑Harold F. Levison, Martin J Duncan.From the Ku iperBelt to Jupiter-Family Comets: The Spatial Distribution of Ecliptic Comets (in English) //Icarus. - Elsevier, 1997. - Vol.127,iss.1. - P.13-32. - doi:10.1006/icar.1996.5637.Archived 19 March 2015.
  24. ↑Dawn: A Journey to the Beginning of the Solar System.Space Physics Center: UCLA ( 2005 ).Date access ed: 24 November 2009.Archived 22 August 2011.
  25. ↑An Overview of the Solar System .The Nine Planets.Date accessed: 2 December 2009.Archived 22 August2011.
  26. ↑ TheOuter Planets - article from theBolshoi Soviet Encyclopaedia.
  27. ↑П.Kulikovsky'sHandbook of Amateur Astronomy- 4th ed. - Moscow.Nauka, 1971. - P. 252. - 635 p. - ISBN 9785458272117Archived 12 March 2017 at theWayback Machine
  28. ↑Amir Alexander.New Horizons Set to Launch on 9-Year Voyage to Pluto and the Kuiper Belt.The Planetary Society ( 2006 ).Date access ed: 2 December 2009.Archived 22 August 2011.
  29. ↑Jump back:123The Final IAU Resolution on the definition of "planet" ready for voting . International Astronomical Union (24 August 2006).Date of access:5 December 2009.Archived 27 February 2017.
  30. ↑Jump back:12Dwarf Planets and their Systems (English).Working Group for Planetary System Nomenclature (WGPSN). U.S. Geological Survey (7 November 2008).Date of access:5 December 2009.Archived 17 August 2011.
  31. ↑Ron Ekers.IAU Planet Definition Committee . International Astronomical Union.Date of access:5 December 2009.Archived from theoriginal on 3 June 2009.
  32. ↑Plutoid chosen as name for Solar System objects like Pluto . International Astronomical Union (11 June 2008).Date of access:5 December 2009.Archived 22 August 2011.
  33. ↑Jump back:1234M. Podolak; J. I. Podolak; M. S.Marley.Further investigations of random models of Uranus and Neptune // Planet . Space Sci. - 2000. - Vol.48. - P.143-151. - doi:10.1016/S0032-0633(99)00088-4.Archived 11 October 2007.
  34. ↑Jump back:123M. Podolak; A. Weizman; M.Marley:Comparative models of Uranus and Neptune // Planet . Space Sci. - 1995. - Vol.43,iss.12. - P.1517-1522. - doi:10.1016/0032-0633(95)00061-5.Archived 11 October 2007
 
This is one tenth of the links to material in the Wikipedia article on the Solar System.
 

Conclusion:

It would take a week to pull all the information about the Solar System that is outlined in the Wikipedia article from ChatGPT. If that's even possible.

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