Top 10 similar words or synonyms for spectral

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Top 30 analogous words or synonyms for spectral

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ထရိုင်ဂူလယ် (ကြယ်စုတန်း) an orange giant of spectral type K0III around 520 light-years distant with a visual magnitude of 8.42. A huge starspot larger than the diameter of the sun was detected on its surface in 1999 by astronomers using Doppler imaging.
မိုင်မို မိုင်မိုနည်းပညာသည် ဘန်းဝစ်ဒ် နှင့် ပါဝါကို တိုးမြှင့်ရန် မလိုပဲ ဒေတာ ထုတ်လွှတ်မှုနှုန်းနှင့် ဆက်သွယ်မှု အကွာအဝေးကို သိသိသာသာ တိုးမြှင့်နိုင်သဖြင့် ကြိုးမဲ့ဆက်သွယ်ရေး စနစ်တွင် အလေးပေးအာရုံစိုက်ခြင်း ခံရသည်။ ထိုသို့ တိုးမြှင့်နိုင်ရသည့် အကြောင်းမှာ စပက်ထရယ် အဖစ်ရှန်စီ (spectral efficiency ) ပိုမိုများပြားသည်က တစ်ကြောင်း၊ ဆက်သွယ်ရေး လမ်းကြောင်း၏ စိတ်ချအားထားရမှုနှင့် လမ်းကြောင်း အပို အများအပြား ရှိမှု တို့ကြောင့် မှေးမှိန်ပျောက်ကွယ်ခြင်း ကို လျှော့ချနိုင်သောကြောင့် ဖြစ်သည်။ ထိုသို့သော ဂုဏ်သတ္တိများကြောင့် မိုင်မိုသည် IEEE 802.11n (ဝိုင်ဖိုင်)၊ 4G ၊ 3GPP Long Term Evolution၊ ဝိုင်မက် ( WiMAX ) နှင့် အိတ်ချ်အက်စ်ပီအေ ပလပ်စ် စသည့်ခေတ်သစ် ကြိုးမဲ့ဆက်သွယ်ရေး စံနှုန်းများ၏ အဓိက အရေးပါသော အစိတ်အပိုင်းတစ်ခု ဖြစ်လာခဲ့သည်။
ထရိုင်ဂူလယ် (ကြယ်စုတန်း) R Trianguli is a long period (Mira) variable that ranges from magnitude 6.2 to 11.7 over a period of 267 days. It is a red giant of spectral type M3.5-8e, lying around 960 light-years away. HD 12545, also known as XX Trianguli, is
ထရိုင်ဂူလယ် (ကြယ်စုတန်း) Three star systems appear to have planets. HD 9446 is a sun-like star around 171 light-years distant that has two planets of masses 0.7 and 1.8 times that of Jupiter, with orbital periods of 30 and 193 days respectively. WASP-56 is a sun-like star of spectral type G6 and apparent magnitude 11.48 with a planet 0.6 the mass of Jupiter that has a period of 4.6 days. HD 13189 is an orange giant of spectral type K2II about 2–7 times as massive as the sun with a planetary or brown dwarf companion between 8 and 20 times as massive as Jupiter, which takes 472 days to complete an orbit. It is one of the largest stars discovered to have a planetary companion.
ထရိုင်ဂူလယ် (ကြယ်စုတန်း) Iota Trianguli is a double star whose components can be separated by medium-sized telescopes into a strong yellow and a contrasting pale blue star. Both of these are themselves close binaries. X Trianguli is an eclipsing binary system that ranges between magnitudes 8.5 and 11.2 over a period of 0.97 days. RW Trianguli is a cataclysmic variable star system composed of a white dwarf primary and an orange main sequence star of spectral type K7 V. The former is drawing off matter from the latter, forming a prominent accretion disc. The system is around 1075 light-years distant.
ထရိုင်ဂူလယ် (ကြယ်စုတန်း) Three stars make up the long narrow triangle that gives the constellation its name. The brightest member is the white giant star Beta Trianguli of apparent magnitude 3.00, lying 127 light-years distant from Earth. It is actually a spectroscopic binary system; the primary is a white star of spectral type A5IV with 3.5 times the mass of our sun that is beginning to expand and evolve off the main sequence. The secondary is poorly known, but calculated to be a yellow-white F-type main-sequence star around 1.4 solar masses. The two orbit around a common centre of gravity every 31 days, and are surrounded by a ring of dust that extends from 50 to 400 AU away from the stars.
ထရိုင်ဂူလယ် (ကြယ်စုတန်း) The second-brightest star, the yellow-white subgiant star Alpha Trianguli (3.41) with a close dimmer companion, is also known as Caput Trianguli or Ras al Muthallath, and is at the apex of the triangle. It lies around 7 degrees north-northwest of Alpha Arietis. Making up the triangle is Gamma Trianguli, a white main sequence star of spectral type A1Vnn of apparent magnitude 4.00 about 112 light-years from Earth. It is around double the size of and around 33 times as luminous as the sun and rotates rapidly. Like Beta, it is surrounded by a dusty debris disk, which has a radius 80 times the distance of the Earth from the Sun. Lying near Gamma and forming an optical triple system with it are Delta and 7 Trianguli. Delta is a spectroscopic binary system composed of two yellow main sequence stars of similar dimensions to the Sun that lies 35 light-years from Earth. The two stars orbit each other every ten days and are a mere 0.1 AU apart. This system is the closest in the constellation to the Earth. Only of magnitude 5.25, 7 Trianguli is much further away at around 280 light-years distant from Earth.
ဆေတန် ၅ ဒုံးပျံ On September 3, 2002, astronomer Bill Yeung discovered a suspected asteroid, which was given the discovery designation J002E3. It appeared to be in orbit around the Earth, and was soon discovered from spectral analysis to be covered in white titanium dioxide paint, the same paint used for the Saturn V. Calculation of orbital parameters identified the apparent asteroid as being the Apollo 12 S-IVB stage. Mission controllers had planned to send Apollo 12's S-IVB into solar orbit, but the burn after separating from the Apollo spacecraft lasted too long, and hence it did not pass close enough to the Moon, remaining in a barely stable orbit around the Earth and Moon. In 1971, through a series of gravitational perturbations, it is believed to have entered in a solar orbit and then returned into weakly captured Earth orbit 31 years later. It left Earth orbit again in June 2003. Another near-earth object, discovered in 2006 and designated 6Q0B44E, may also be part of an Apollo spacecraft.