बृहस्पतिग्रह
नेपाली विकिपीडियाबाट
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Designations
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| Pronunciation | |||||||||||||||||||||||
| Adjective | Jovian | ||||||||||||||||||||||
| Epoch J2000 | |||||||||||||||||||||||
| Aphelion | ८१६,५२०,८०० km (५.४५८१०४ AU) | ||||||||||||||||||||||
| Perihelion | ७४०,५७३,६०० km (४.९५०४२९ AU) | ||||||||||||||||||||||
| Semi-major axis | ७७८,५४७,२०० km (५.२०४२६७ AU) | ||||||||||||||||||||||
| Eccentricity | 0.048775 | ||||||||||||||||||||||
| परिभ्रमण अवधि | 4,331.572 days 11.85920 yr 10,475.8 Jupiter solar days[४] |
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| परिभ्रमण अवधि | 398.88 days[५] | ||||||||||||||||||||||
| परिभ्रमण गति | 13.07 km/s[५] | ||||||||||||||||||||||
| Mean anomaly | 18.818° | ||||||||||||||||||||||
| Inclination | 1.305° to Ecliptic 6.09° to Sun's equator 0.32° to Invariable plane[६] |
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| Longitude of ascending node | 100.492° | ||||||||||||||||||||||
| Argument of perihelion | 275.066° | ||||||||||||||||||||||
| उपग्रह | 63 | ||||||||||||||||||||||
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Physical characteristics
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| औशत अर्धब्यास | 69,911 ± 6 km[७][८] |
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| भूमध्यरेखीय अर्धब्यास | 71,492 ± 4 km[७][८] 11.209 Earths |
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| ध्रुवीय अर्धब्यास | 66,854 ± 10 km[७][८] 10.517 Earths |
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| Flattening | 0.06487 ± 0.00015 | ||||||||||||||||||||||
| सतहको क्षेत्रफल | 6.21796×1010 km2[८][९] 121.9 Earths |
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| आयतन | 1.43128×1015 km3[५][८] 1321.3 Earths |
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| पिण्ड | 1.8986×1027 kg[५] 317.8 Earths 1/1047 Sun[१०] |
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| औशत घनत्व | 1.326 g/cm3[५][८] | ||||||||||||||||||||||
| Equatorial surface gravity | 24.79 m/s2[५][८] 2.528 g |
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| Escape velocity | 59.5 km/s[५][८] | ||||||||||||||||||||||
| परिक्रमण अवधि | 9.925 h[११] (9 h 55 m 30 s) | ||||||||||||||||||||||
| Equatorial rotation velocity | 12.6 km/s 45,300 km/h |
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| अक्षको झुकाव | 3.13°[५] | ||||||||||||||||||||||
| North pole right ascension | 268.057° 17 h 52 min 14 s[७] |
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| North pole declination | 64.496°[७] | ||||||||||||||||||||||
| Albedo | 0.343 (Bond) 0.52 (geom.)[५] |
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| Surface temp. 1 bar level 0.1 bar |
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| Apparent magnitude | -1.6 to -2.94[५] | ||||||||||||||||||||||
| Angular diameter | 29.8" — 50.1"[५] | ||||||||||||||||||||||
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Atmosphere[५]
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| वायुमण्डलीय चाप | 20–200 kPa[१२] (cloud layer) | ||||||||||||||||||||||
| Scale height | 27 km | ||||||||||||||||||||||
| वायुमण्डलीय तत्वहरू |
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भोयजर १ बाट लिईको बृहस्पतिग्रहको तस्बीर
बृहस्पतिग्रह सौर्यमण्डको सबैभन्दा ठूलो र सूर्यबाट पाँचौं ग्रह हो। ग्याँसबाट मात्रै बनेकोले, त्यसलाई ग्याँस पिण्ड भन्छन्। सौर्यमण्डलको अरु सात ग्रहको पिण्ड जम्म गरेपनि, बृहस्पतिग्रहको पिण्ड झन बढी हुन्थ्यो।
सन् २००३मा बृहस्पतिको वरिपरि घुमिरहेको ६३वटा चन्द्रमा पत्ता लगाइसकेको थिए। त्यीमाध्य सबभन्दा ठूलो ४वटा चन्द्र वैज्ञानिक गालिलेयोले पत्ता लागेकोले, गालिलेयी चन्द्रमा भन्छन्। तिनीका नाम आयो, युरोपा, ग्यानिमिड र कलिस्टो हुन्।
बृहस्पतिग्रह ठूलो भएर त्यसको वायु-मण्डल गहिरो गएर उच्च चाप हुन्छ। अन्तरिक्षयान बृहस्पतिभित्र पस्यो भने, एक छिनमै किचिन्थ्यो। त्यसकारणले बृहस्पतिको वायु-मण्डलभित्र के के छ भनेर थोरै थाहा छ।
बृहस्पतिको पतलो चक्क छ।
[सम्पादन गर्ने] थप जानकारीका लागि हेर्नुहोस्
[सम्पादन गर्ने] सन्दर्भ
- ↑ Jupiter, entry in the Oxford English Dictionary, prepared by J. A. Simpson and E. S. C. Weiner, vol. 8, second edition, Oxford: Clarendon Press, 1989. ISBN 0-19-861220-6 (vol. 8), ISBN 0-19-861186-2 (set.)
- ↑ Yeomans, Donald K. (2006-07-13), "HORIZONS System" — At the site, go to the "web interface" then select "Ephemeris Type: Elements", "Target Body: Jupiter Barycenter" and "Center: Sun".
- ↑ Orbital elements refer to the barycenter of the Jupiter system, and are the instantaneous osculating values at the precise J2000 epoch. Barycenter quantities are given because, in contrast to the planetary centre, they do not experience appreciable changes on a day-to-day basis from to the motion of the moons.
- ↑ Seligman, Courtney, "Rotation Period and Day Length"
- ↑ Cite error: Invalid
<ref>tag; no text was provided for refs namedfact - ↑ "The MeanPlane (Invariable plane) of the Solar System passing through the barycenter", 2009-04-03 (produced with Solex 10 written by Aldo Vitagliano; see also Invariable plane)
- ↑ ७.० ७.१ ७.२ ७.३ ७.४ Seidelmann, P. Kenneth (2007), "Report of the IAU/IAGWorking Group on cartographic coordinates and rotational elements: 2006", Celestial Mechanics and Dynamical Astronomy 90(3): 155–180, doi: 10.1007/s10569-007-9072-y , <http://adsabs.harvard.edu/doi/10.1007/s10569-007-9072-y>. Retrieved on २८ अगस्त २००७
- ↑ ८.० ८.१ ८.२ ८.३ ८.४ ८.५ ८.६ ८.७ Refers to the level of 1 bar atmospheric pressure
- ↑ "Solar System Exploration: Jupiter: Facts & Figures", NASA, 7 May 2008
- ↑ "Astrodynamic Constants", 2009-02-27
- ↑ Seidelmann, P. K.; Abalakin, V. K.; Bursa, M.; Davies, M. E.; de Burgh, C.; Lieske, J. H.; Oberst, J.; Simon, J. L.; Standish, E. M.; Stooke, P.; Thomas, P. C. (2001), "Report of the IAU/IAG Working Group on Cartographic Coordinates and Rotational Elements of the Planets and Satellites: 2000"
- ↑ Anonymous (March 1983), "Probe Nephelometer", Galileo Messenger (NASA/JPL) (6), <http://www2.jpl.nasa.gov/galileo/messenger/oldmess/2Probe.html>. Retrieved on १२ फेब्रुअरी २००७
| सौर्य परिवार | |||||||
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| सूर्य • Heliosphere |
ग्रहहरु ☾ = उपग्रह(s) ∅ = rings |
बुधग्रह | शुक्रग्रह | पृथ्वी ☾ | मंगलग्रह ☾ | ||
| बृहस्पतिग्रह ☾ ∅ | शनिग्रह ☾ ∅ | अरुणग्रह ☾ ∅ | वरुणग्रह ☾ ∅ | ||||
| क्षुद्रग्रहहरु | सेरेस | यम ☾ | हुमेआ ☾ | मेकमेक | |||
| Eris ☾ | |||||||
| Small Solar System bodies |
शिशुग्रहहरु (साना ग्रहहरु) |
Groups and families: Vulcanoids · Near-Earth asteroids · Asteroid belt Jupiter Trojans · Centaurs · Neptune Trojans · Asteroid moons · Meteoroids · Pallas · Juno · Vesta · Hygiea · |
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| See also the list of asteroids, and the meaning and pronunciation of asteroid names. | |||||||
| Trans- Neptunians |
Kuiper belt – Plutinos: Orcus · Ixion – Cubewanos: 2002 UX25 · Varuna · 1992 QB1 · 2002 TX300 · Quaoar · Huya · 2002 AW197 |
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| Scattered disc: 2002 TC302 · 2004 XR190 · Sedna | |||||||
| पुच्छ्रेताराहरु | Lists of periodic and non-periodic comets · Damocloids · Hills cloud · Oort cloud | ||||||
| See also Geology of solar terrestrial planets, astronomical objects, the solar system's list of objects, sorted by radius or mass, and the Solar System Portal | |||||||