What is the translation of " VARIABLE STAR " in Slovenian?

• spremenljiva zvezda
• zvezda spremenljivka
• variable star

Examples of using Variable star in English and their translations into Slovenian

In short, we have a variable star.".
Na kratko- imamo zelo spremenljivo zvezdo.«.

Another youthful variable star, V1023 Tauri, can be spotted on the left.
Levo lahko opazimo še eno mladostno spremenljivo zvezdo, V1023 Bika.

His special interest was variable stars.
Največ se je posvečal spremenljivim zvezdam.

The prototypical example is the variable star T Tauri, visible as the bright orange star near the image center.
Vzorčni primer je spremenljiva zvezda T Bika, ki jo vidimo kot svetlo oranžno zvezdo blizu središča slike.

Did you know the Sun is a variable star?
Ali ste vedeli, da je naše Sonce spremenljiva zvezda?

Note that variable stars have their own naming convention which, while being somewhat convoluted, is at least consistent across the astronomical community.
Upoštevajte, da imajo spremenljive zvezde svoj način poimenovanja, ki, medtem ko je nekoliko zapletena, je vsaj dosleden prek astronomske skupnosti.

Scientists have found nine new variable stars.
Znanstveniki so odkrili devet novih spremenljivih zvezd.

Variable star R Aquarii is actually an interacting binary star system, two stars that seem to have a close, symbiotic relationship.
Spremenljiva zvezda R Aquarii(R Vodnarja) je v resnici interagirajoča dvojna zvezda, v kateri imata zvezdi tesno, simbiotično zvezo.

Retrieved 12 September 2013.↑"Eta 1Hydri- Variable Star".
Pridobljeno dne 12 September 2013. ↑"Eta 1Hydri- Variable Star".

Within are extremely young variable stars V633 Cas(top) and V376 Cas.
Znotraj sta zelo mladi spremenljivi zvezdi V633 Cas(zgoraj) in V376 Cas.

Retrieved 12 September 2013.↑"Gamma Hydri- Variable Star".
Pridobljeno dne 12 September 2013. ↑"Gamma Hydri- Variable Star".

Observations of NGC 1309's recent supernova and Cepheid variable stars contribute to the calibration of the expansion of the Universe.
Opazovanja nedavne supernove v NGC 1309 in spremenljivih zvezd Kefeid so prispevala k kalibraciji širjenja vesolja.

The bright bluish nebula below and left of center is NGC 1999, a dusty cloud reflecting light from an embedded variable star.
Svetla modrikasta meglica spodaj levo od središča je NGC 1999, prašen oblak, ki odbija svetlobo iz spremenljive zvezde v oblaku.

Later, discovering that the one near the upper right corner was actually a type of variable star known as a cepheid, he crossed out the"N" and wrote"VAR!".
Kasneje, ko je odkril da je zvezda blizu zgornjega desnega kota(označena s črticama) v resnici spremenljiva zvezda, poznana kot kefeida, je prečrtal"N" in napisal"VAR!".

In fact, RS Pup is a Cepheid variable star, a class of stars whose brightness is used to estimate distances to nearby galaxies as one of the first steps in establishing the cosmic distance scale.
Pravzaprav je RS Krma spremenljiva zvezda tipa kefeide, razreda zvezd, katerih svetlost se uporablja za oceno razdalj do bližnjih galaksij, kot enega prvih korakov za določitev vesoljske lestvice razdalj.

It shows the light curve of the variable star YZ Boo.
Opazovanje za projekt"Svetlobna krivulja spremenljive zvezde YZ Boo".

After detecting a sudden outburst from the star in 2002, astronomers have followed the flash expanding at the speed of light through pre-existing dust clouds surrounding the reddened variable star.
Potem, ko so leta 2002 zaznali nenaden izbruh zvezde, so astronomi zasledovali blisk, ki se je s svetlobno hitrostjo širil skozi že prej obstoječi prašni oblak, ki je obdajal pordečelo zvezdo spremenljivko.

Adrift in Orion's stellar nursery and still in its formative years, variable star LL Orionis produces a wind more energetic than the wind from our own middle-aged Sun.
Povezana z Orionovo zvezdno porodnišnico in še vedno v letih oblikovanja, spremenljiva zvezda LL Oriona tvori veter, ki je bolj energetski od vetra našega Sonca v srednjih letih starosti.

At the edge of the Orion molecular cloud complex some 1,500 light-years distant, NGC 1999 is illuminated by the embedded variable star V380 Orionis.
Na robu kompleksa Orionovih molekularnih oblakov, oddaljenih kakih 1.500 svetlobnih let, meglico NGC 1999 osvetljuje v oblak zavita spremenljiva zvezda V380 Oriona.

Adrift in Orion's stellar nursery and still in its formative years, variable star LL Orionis produces a wind more energetic than the wind from our own middle-aged Sun.
Gnana od Orionove zvezdne porodnišnice in še vedno v procesih nastajanja, spremenljiva zvezda LL Oriona ustvarja vetrove, ki so bolj energetski od vetrov iz našega srednjih let starega Sonca.

These names include Bayer designations such as Alpha Centauri, Flamsteed designations such as 61 Cygni, and variable star designations such as RR Lyrae.
Ta imena vsebujejo Bayerjevo poimenovanje, kot je α Kentavra(α Cen), Flamsteedovo poimenovanje, kot je 61 Laboda(61 Syg) in poimenovanja spremenljivih zvezd kot je RR Lire(RR Lyr).

(Betelgeuse is a variable star and can at its maximum occasionally outshine Rigel.)[6] Bayer then repeated the procedure for the stars of the 2nd magnitude, labeling them from gamma through zeta in"top-down"(north-to-south) order.
(Betelgeza je zvezda spremenljivka in le včasih preseže sij Rigla.) Bayer je kasneje ponovil postopek za zvezde 2. magnitude, kjer je določil zvezde od Game pa vse do Zete od severa proti jugu.

Expanding light echoes continue to illuminate the dusty environs of V838 Monocerotis, mysterious variable star near the edge of our Galaxy.
Razširjajoči svetlobni odmevi še vedno osvetljujejo prašno okolico V838 Enoroga, skrivnostno zvezdo spremenljivko blizu roba naše Galaksije.

HD 316285 is listed in the General Catalogue of Variable Stars as a variable Be star with a range of about one tenth of a magnitude.[15] The International Variable Star Index classifies it as an S Doradus variable[16] and it is considered to be a candidate Luminous Blue Variable..
HD 316285 je na seznamu Splošnega kataloga spremenljivk kot zvezda spremenljivka berilijevega tipa, z nihanjem okoli 1 desetino magnitude.[1] Mednarodni katalog zvezd spremenljivk jo je uvrstil v kategorijo spremenljivk S Zlate ribe[2] in je kandidat za svetle modre spremenljivke..

Flamsteed designation Gould designation Lists of constellations Star catalogue Star designation Table of stars with Bayer designations Variable star designation.
Flamsteedovo poimenovanje Gouldovo poimenovanje Seznam ozvezdij Zvezdni katalog Zvezdno poimenovanje Tabela Bayerjevih zvezd Poimenovanje zvezdnih spremenljivk.

It is chemically peculiar star that displays an anomalous abundance of the element silicon in its spectrum.[1] This is a suspected variable star of the type known as Alpha² Canum Venaticorum.[2] There is a magnitude 9.86 companion star at an angular separation of 2.30″ along a position angle of 131°.[3].
Zaradi anomalistične pogostosti elementa silicija v svojem spektru je kemijsko posebna zvezda.[1] Verjetno je zvezda spremenljivka tipa Alfe2 Lovskih Psov.[2] Obkroža jo tudi spremljevalec z magnitudo 9,86 na kotni razdalji okoli 2,30 ˝ v pozicijskem kotu 131°.[3].

Identification of stars within a given constellation includes the use of Bayer designations such as Alpha Centauri, Flamsteed designations such as 61 Cygni, and variable star designations such as RR Lyrae.
Ta imena vsebujejo Bayerjevo poimenovanje, kot je α Kentavra(α Cen), Flamsteedovo poimenovanje, kot je 61 Laboda(61 Syg) in poimenovanja spremenljivih zvezd kot je RR Lire(RR Lyr).