(ST reference: Star Charts) ST reference: Star Charts Mu Virginis article at Wikipedia, the free encyclopedia. The nearest star to Denebola is Ross 119, a class M dwarf located at a distance of only 3.6 light years from Denebola. Based on the star's spectral, the stars temperature is between 2,400.00 and 3,700.00 degrees kelvin. Star system - Mufrid [INARA] For example, in a solar eclipse the moon gets between the sun and . W Virginis - Universe Guide The strength of the star's spectral . We have also calculated the bolometric flux from published measurements which, combined with the angular diameter . Vindemiatrix (Epsilon Virginis) | Star Facts 'Golembiewski, Billingsly & Jaeger proposed three types of change - alpha, beta and gamma.' 'G proteins consist of three subunits, alpha, beta, and gamma, and exist in many different classes.' 'There are three major caseins - alpha, beta and kappa - that differ by their size.' 'There are several types of simple proteins known as globulins in the blood: alpha, beta, and gamma . It has a mass 2.64 times that of the Sun and a radius 10.6 times solar. Gamma Virginis is a binary star, consisting of two stars of approximately equal apparent magnitudes 3.65 and 3.56, and of spectral type F0V. Jump to navigation Jump to search. Beta Virginis, a name Latinised from β Virginis, is a star in the equatorial constellation of Virgo.It has the proper name Zavijava (/ ˌ z æ v ɪ ˈ dʒ æ v ə /), and, despite its designation 'beta', is the fifth-brightest star in Virgo with an apparent visual magnitude of 3.604. Since the constellation boundaries were fixed it belon. Drawn by Jim Thomas on 19 June, 2006. Secular Behavior In Multi-planet Systems: 61 Virginis, 55 Cancri, Etc. Spica (Alpha Virginis): Star System, Name, Constellation ... Denebola (Beta Leonis): Star Type, Facts, Name, Location ... The Host Stars of Extrasolar Planets Have Normal Lithium Abundances. Achernar Alpha Eridani 144 ly 9 B type blue dwarf or giant 18. This paper presents the modeling of the F9 V star beta Virginis based on seismological measurements. Being a Beta Cephei-type variable, the primary star's luminosity varies slightly over a period of 0.1738 days. star in the constellation Virgo. The star Beta Pictoris is an A type star, pale blue. The star system is notable for possessing a large disk of material, in which planets might be located. Based upon parallax measurements, it is located at a distance of about 198 light-years (61 parsecs) from the Sun. Zavijava; Statements. What type of star is Beta Virginis? Zubeneschamali is a hot blue hydrogen-fusing star of the spectral type B8 V. It has a mass 3.5 times that of the Sun and a radius 4.9 times solar. Fun fact: we deliver faster than Amazon. Beta Sagittarii (Arkab) is a binary star system in the constellation Sagittarius.β¹ Sagittarii: Is a type B9V star. The primary star is 10 times heavier than the sun. A two-star system around 260 light-years of earth. Auwa - Delta Virgins. Vindemiatrix / Epsilon Virginis is a giant star, with a yellow-hued glow of a G-type star, and with a stellar classification of G8 III. Own navigation aid is integrated in big categories. Aliens / U.F.O. It is unusual as it is one of the few planets outside our Solar System that has been . Appropriately ranking . The star is a slow spinner. Bayer placed the star in constellations Taurus as well as Auriga. Facts. If there is life on any Earth-type planet . F-type main-sequence star. Gamma Virginis has a visual magnitude of 2.74 and is approximately 38.1 light years distant. Mu Virginis was a binary star system consisting of two type F white stars. Many neutral metals (Fe I, Mg I, Ca I) weakly appear, but the spectrum overall is dominated by the hydrogen series. Apart from Ursa Major that is circumpolar, constellations that are now visible include Leo, Boötes, Hydra . beta Orionis (B8Ia) tau Scorpii (B0V) alpha Virginis (B1III) alpha Leonis (B7V) A: Very strong Balmer hydrogen lines, which peak in strength in Type A2, and the disappearance of He I. They orbit each other at about 90 km/sec (56 m/sec), and complete one orbit every four days . Beta Virginis is called ~, from an Arabic name meaning 'the angle'; in the Almagest, Ptolemy located this star . Closest B type stars : . Beta Virginis (also known as Zavijava) is a star system, a trinary star located in the space of the galaxy's Beta Quadrant. The spectrum shows a radial velocity variation with the same period, indicating that the surface of the star is regularly pulsating outward and then contracting. There are 133 stars marked on this map. The advent of spring in the Northern Hemisphere is slowly ushering in improved seeing conditions, and along with it, a few seasonal constellations that had been out of view for some time. The distance to this star is 35.7 light-years based on parallax, and it is drifting further away with a radial . PV Telescopii variables. (ST reference: Star Charts) Phi Virginis article at Wikipedia, the free . Your anaconda definitely wants some. Its approximate distance is 35.65 light-years. Alpha Virginis - Type d'objet: Variable Star of beta Cep type, Étoile, Double or multiple star, Infra-Red source, Étoile binaire, UV-emission source, Variable Star, X-ray source On the N.A.S.A. It is a "Beta Cephei variable" which means that the variation in its brightness is due to . The . Its visual magnitude is 2.71 and its approximate distance is 38.1 light-years. With an effective temperature of 5,086 K, it is 77 times more luminous than the Sun. Delta Virginis belongs to a small group to the west of Spica called the "awwa," which may represent some kind of barking dogs (or it may not), composed of Zavijava (Beta Vir), Porrima (Gamma), Vindemiatrix (Epsilon), Zaniah (Eta), and our otherwise un-named Delta. The Alpha Virginis star system is a massive source of X-rays. It is 250 light years distant from our Solar System.Like Regulus, Spica is regularly occulted by the Moon and less frequently so by the various planets of the . W Virginis brightness ranges from a magnitude of 10.747 to a magnitude of 9.652 over its variable period. Delta . It consists of two almost identical main sequence stars at a distance of about 38 light-years . Below is a table of brief descriptions of variability types; more complete descriptions can be found in Volume 1 of the General Catalog of Variable Stars, 4th Edition (Kholopov et al. Together with Beta, Eta, Delta and Epsilon Virginis, the star formed an asterism known as Barker, or Al ʽAwwāʼ. Emeritus of Astronomy, University of Illinois Scroll down for previous stars, Places to Go, and the complete stellar archive. well, in answer to that, there's a question to you. [2] With an orbital period of 168.93 years, [3] it was an easy object for amateur astronomers until the beginning of the 1990s, but in 2011 the smaller apparent distance between the stars requires a larger . HIP 78521 b. Hubble Classification. This means it is a blue giant/supergiantβ² Sagittarii: Is a type F2III. A planet, named Beta Pictoris b, was observed in 2008 using ESO's NACO instrument on the Very Large Telescope (VLT). You can the solar system for NY Virginis at N.A.S.A. The star is a eclipsing binary sys Beta Lyrae (Sheliak) variable type which means that its size changes over time. The Beta Virgins' traditional name is Zavijava and the fifth brightest star. Contested by Edmund Mahon, Zachary Hudson. 1, 2019, below have all appeared as a Star of the Week on . Its variable/pulsating period lasts for 1 . Its projected rotational velocity is 58.8 km/s. There are roughly 1400 star systems within this volume of space containing 2000 stars, so this map only shows . The Variable Type is usually named after the first star of that type to be spotted. Epsilon Virginis (ε Virginis, abbreviated Epsilon Vir, ε Vir), formally named Vindemiatrix / v ɪ n d iː m i ˈ eɪ t r ɪ k s /, is a star in the zodiac constellation of Virgo.The apparent visual magnitude of this star is +2.8, making it the third-brightest member of Virgo.Based upon parallax measurements made during the Hipparcos mission, Vindemiatrix lies at a distance of about 109.6 . Star type. STARS presents a comprehensive suite of pages that tell the stories of stars and their constellations.The stars listed prior to January. Rho Virginis is a star system, a binary star in the space of the Romulan Star Empire, located in the galaxy's Beta Quadrant. The smaller the magnitude, the brighter the star. Sarpeidon - Also known as Beta Niobe I, this class M planet was visited by the USS Enterprise in 2269 hours before its star, Beta Niobe, went supernova. The Enterprise crew discovered that the natives of the world had escaped their fate by time traveling to their world's past, using a time-travel device called an atavachron. Language Label Description Also known as; English: Beta Virginis . 3. They are at their brightest during minimum contraction. Try that ;-) Wiki User. Exclude . The star is a very fast spinner, with a . Beta Virginis is a yellowish star that is brighter, more massive, and further evolved than our Sun, Sol. The only star in our sample for which we detected pulsations is η Orionis; its orbital period is about twice that of α Virginis. & Astrophys., 525, A65, 6 pp paper preprint. The star's estimated age is 560 million years . This binary consists of two type A light blue stars in the constellation of Virgo, located 118 light-years from Earth. Like other main-sequence stars, a G-type main-sequence star is converting the element . Tau Bootis (Edmund Mahon) Shoujeman (Zachary Hudson) Info updated. Denebola - β Leonis (Beta Leonis) Denebola is the second brightest star in Leo and the 61st brightest star in the sky.It is a main sequence star with the stellar classification A3 V. It has an apparent magnitude of 2.113 and is approximately 35.9 light years distant from Earth.. Denebola Incident Great Whale ISO, The Pacifican Slang Porrima Virginis Combine, The Gamma Virginis is a binary star known as Porrima. Delta Vir is one of the sky's rather few naked-eye class M red giants, and a coolish one (class M3) at that. Information as of: 11.2020 Source Wikipedia (Authors [History]) License : CC-BY-SA-3. Beta Virginis belongs to the spectral class F9 V. It is only 35.65 light-years distant from the Sun and is only the fifth brightest star in the constellation. 4. IFunny is fun of your life. Those who show natural trading ability and genuine motivation will be invited to our office for an interview. The two components of the binary system are too close together to be resolved optically, with the average distance between the two stars only about 18 million kilometers (11 million miles). 2000 RYAN S MNRAS, 316, L35 paper arxiv. . Porrima - Gamma Virginis. 10 Nov 2021, 12:20am. This is a map of every star within 50 light years visible with the naked eye from Earth. Iota Virginis (Syrma) is a star in the constellation Virgo.It is yellow dwarf with a spectral class of F6 which means it will appear as yellow white.It is located about 70 light years from us. Gamma Virginis ( γ Virginis, abbreviated Gamma Vir, γ Vir ), officially named Porrima / ˈpɒrɪmə /, is a binary star system in the constellation of Virgo. With a projected rotational velocity of 2.3 km/s, it takes 173 days to complete a rotation. [9] Despite being the beta star of the constellation Virgo it is only the fifth star in order of brightness.. Physically, Beta Virginis is larger and more massive than the Sun, and is comparatively metal-rich (that is, it has a higher preponderance of . 1 reference. HD 126525 b. HO Librae g. Constellations. Spica can be located by following the arc of the Big Dipper's handle, formed by the bright Alkaid, Mizar and Alioth. We provide a small, live cryptocurrency account for you to participate from home. (beta) Cephei variables (or beta Canis Majoris variables, as these stars are generally called in Europe) undergo short period pulsations in the order of 0.1 - 0.6 days with an amplitude of 0.01 - 0.3 magnitudes. Beta Pictoris (β Pic, β Pictoris) is a main sequence star in the constellation of Pictor. No. Based on the star's spectral type of M5.5V C , FL Virginis's colour and type is red main sequence star. This trinary consists of two type F white stars with an type A blue-white companion in the constellation of Virgo, located 35 light years from Earth, in the general vicinity of system p Eridani, Iota Horologii, Kaleb and Porrima. Zavijava - β Virginis (beta Virginis) Zavijava, also designated as β Virginis (beta Virginis), is a multiple main-sequence star in the constellation of Virgo . Those type of names that use letters from the Greek alphabet are the technical names used by astronomers. An Earth-type planet could have liquid water in a stable orbit centered around 3.5 AU (within a predicted habitable zone ranging between 2.3 and 4.8 AUs) from Star A -- between the orbital distances of the Main Asteroid Belt and Jupiter in the Solar System (NASA Stars and Exoplanet Database). The star is the brightest star of the Virgo constellation and the 15th brightest star overall in the night sky. So many stars have their arabic or latin names included. The names of stars and . The two component stars of Beta Lyrae systems are quite heavy (several solar masses (M ☉) each) and extended (giants or supergiants). The star is a pulsating W Virginis Stars, A variable type which means that its size changes over time. It has a luminosity 2,254 times that of the Sun. STARS and STARS OF THE WEEK Star Count: 950 Created by Jim Kaler, Prof. Asset gained on victory: Quimby Station. After correcting for limb darkening and combining with the revised Hipparcos parallax, we derive a radius of 1.703 +/- 0.022 R_sun (1.3%). Using the Geneva evolution code including rotation and atomic diffusion, we find that two . Both stars in the Gamma Virginis system are of the spectral type F0V and have similar visual magnitudes, 3.65 and 3.56. In comparison, the distance from the Sun to the nearest star system, BCEP Variables of the Beta Cephei type (Beta Cep, Beta CMa), which are pulsating O8-B6 I-V stars with periods of light and radial-velocity variations in the range of 0.1 - 0.6 days and light amplitudes from 0.01 to 0.3 mag in V. The light curves are similar in shape to average radial-velocity curves but lag in phase by a quarter of the period, so that maximum brightness corresponds to maximum . Variable Type. Beta Cephei Stars Beta Cephei Stars and Their Relatives: Winter 2005 Cepheids RS Pup: January 2011 TU Cas: Fall 2005 W Virginis: Spring 2003 X Cygni: September 2002 Zeta Geminorum: March 2002 Delta Cephei: September 2000 Delta Scuti Variables Delta Scuti and the Delta Scuti Variables: Summer 2004 Mira Stars RU Vir: April 2007 Khi Cygni . This binary consists of two type G yellow stars in the constellation of Virgo, located 135 light-years from Earth, in the general vicinity of Epsilon Librae, Alpha Indi, and the space of the Typhon Expanse. Spring Constellations of the Northern Hemisphere. New Luna, a microjovian in the Beta Virginis system: These worlds have masses between 0.03 and 0.08 that of Jupiter and are intermediate in size between Superterrestrial worlds and the larger gas giants. infrared source. Because of its moderate brightness, Zavijava should be easily visible from locations with dark skyes, while it can be barely visible, or not visible . Zavijava / Beta Virginis Facts (Type, Distance, Magnitude, Age, Colour, Luminosity, Location & more) . Beta Virginis (Q14201) From Wikidata. Acrux Alpha Crucis 320 ly 13 Multiple blue giants 22. Delta Virginis belongs to a small group to the west of Spica called the "awwa," which may represent some kind of barking dogs (or it may not), composed of ~ (Beta Vir), Porrima (Gamma), Vindemiatrix , Zaniah (Eta), and our otherwise un-named Delta. Albedo and Reflection Spectra of Extrasolar Giant Planets 2000 SUDARSKY D . Vindemiatrix is a yellow giant of the spectral type G8 III. star in the constellation Virgo. imported from Wikimedia project. Distance to FL Virginis. Updated. El Nath Beta Tauri 131 ly 27 Be type shell star 17. Most likely, it may be a binary star. This star is rotating . Changes: Only links which lead directly or redirect to an article or a category were taken over. Newsletter. Stars in this class are helium supergiants with a period of 0 . Spica, or Alpha Virginis, is another example in the constellation Virgo. Star Beta is a diversified Proprietary Trading Firm trading in multiple asset classes such as Futures, Stocks, Bonds, Commodities and Currencies. Beta Pictoris. Menu. & Astrophys., 356, 213 paper. The stars are only 8 light years apart. Many gaseous protoplanets of this kind form very early on in the development of a planetary system, but most are incorporated by larger objects, ejected by larger objects into interstellar . Requirements: Completion (or final term) of Tertiary education. The . Beta Pictoris 2.10 A5 Gamma Virginis 1.70 F0 Eta Arietis 1.29 F5 Beta Comae Ber 1.10 G0 Alpha Mensae 0.93 G6 70 Ophiuchi A 0.78 K0 61 Cygni A 0.69 K5 Gliese 185 0.47 M0 EZ Aquarii A 0.21 M5 BD63137 0.35 Feige41 4.80 HD6111 0.99 HD17647 0.89 HD23733 1.75 HD24189 1.17 HD27685 1.08 SAO81292 0.18 HD35619 20.1 Spectral Classification of Stars 4. It is a main sequence star of the spectral type B2V. 1985), and in the documentation for the machine-readable version (Warren 1988). But some stars can vary hugely. ∙ 2012-04-30 16:56:46. We also operate one of the largest Cryptocurrency . The system consists of a binary pair designated . instance of. SubJovian Type ~ (Beta Virginis) . The primary is classified as a Beta Cephei type variable star that varies in brightness over a 0.1738 day period. Sarpeidon V - Heavily fortified headquarters planet of the . A Comprehensive Characterization of the 70 Virginis Planetary System 2015 KANE S., BOYAJIAN T., HENRY G., FENG Y . Factions updated. NS Virginis brightness ranges from a magnitude of 9.129 to a magnitude of 8.775 over its variable period. System Summary. Zavijava visual magnitude is 3.61. 2000 GIMENEZ A. Astron. Lớn hơn và to hơn Mặt trời, nó tương đối giàu kim loại (nghĩa là nó có độ ưu việt cao hơn của các nguyên . Bellatrix Gamma Orionis 243 ly 26 B type blue giant 19. site. Such a planet would have an orbital period around 4.6 years. Wolf 562 Major Inc: Elections against GQ Virginis General Corporation in LTT 5455 ︎ is pending. The barycentric motion of exoplanet host stars: Tests of solar spin-orbit coupling 2010 PERRYMAN M. & SCHULZE-HARTUNG T. Astron. Spica Alpha Virginis 260 ly 16 Blue giant binary 20. Images, GIFs and videos featured seven times a day. A variable star is a star that is sometimes brighter or dimmer. W Virginis variables Main article: W . Planets. Phi Virginis (also known as 105 Virginis) is a star system, a binary star in the space of the galaxy's Beta Quadrant. For M-type stars displaying ZrO bands, the M types are followed, with or without parentheses, by the type "S"; (4) Orion variables displaying characteristic T Tauri features contain the letter "T" in parentheses following their spectral types; (5) The catalog remarks sometimes report the spectral types for S stars at maximum light according to the new system described by Keenan and Boeshaar . In 1983, before the confirmed . It is about 11 times the mass of the sun, 7.8 times the diameter, and about 260 light-years away. (ST reference: Star Charts) ST reference: Star Charts Rho Virginis article at Wikipedia, the free encyclopedia. Stars within 50 light years . Spica, or Alpha Virginis is the brightest star in Virgo with an apparent magnitude of 0.97. Spica or Alpha Virginis (Alp Vir) is the brightest naked eye star in the constellation Virgo. Beta Virginis is located about 35.6 light-years (ly) away from our Sun, Sol. This . Abstract: We have used the Sydney University Stellar Interferometer (SUSI) to measure the angular diameter of the F9 V star beta Virginis. 'Golembiewski, Billingsly & Jaeger proposed three types of change - alpha, beta and gamma.' 'G proteins consist of three subunits, alpha, beta, and gamma, and exist in many different classes.' 'There are three major caseins - alpha, beta and kappa - that differ by their size.' 'There are several types of simple proteins known as globulins in the blood: alpha, beta, and gamma . Mu Virginis was located in the galaxy's Beta Quadrant in the space visible from Earth in the constellation of Virgo. site, it refers to the star as a O star although in Hipparcos library, it is classed as B star. HD 122430 b. HO Librae. Both stars in the Gamma Virginis system are of the spectral type F0V and have similar visual magnitudes . Type_of_Variability Abbreviation for the possible type of variability of the star. Delta Virginis (δ Virginis, abbreviated Del Vir, δ Vir), formally named Minelauva / ˌ m ɪ n ə ˈ l ɔː v ə /, is a star in the zodiac constellation of Virgo.With an apparent visual magnitude of 3.4, this star is bright enough to be seen with the naked eye. We have also calculated the bolometric flux from published measurements which, combined with the angular diameter, implies an . With an effective temperature of 12,300 K, Zubeneschamali shines with 130 solar luminosities. One of the two goddesses of prophecy known as the Carmenae is called Porrima. The Parallax of the star is given as 227.90000 which gives a calculated distance to FL Virginis of 14.31 light years from the Earth or 4.39 parsecs. ubvy Photometry of stars with planets. Vindemiatrix has an apparent magnitude of +2.8, and an absolute magnitude . After correcting for limb darkening and combining with the revised Hipparcos parallax, we derive a radius of 1.703 +/- 0.022 R_sun (1.3%). Most stars have only very small differences in brightness, like the Sun. The radius is derived from the star's angular diameter, measured at 0.801 milliarcseconds in 2009. HD 122303. English Wikipedia. (ST reference: Star Charts) This system's . Star type. It is about . This answer is: . The recruitment process will involve a two week online assessment. There are generally two types of variable stars: A star being eclipsed, where the changes in brightness are from perspective, are called extrinsic variables. 1 reference. The Sombrero Galaxy is located in Virgo, and we can find it 11.5 degrees to the west of Spica, 5.5 degrees northeast of Eta Corvi in Corvus constellation, just near the border between Virgo and Corvus . It lies at the western edge (1:50:41.7+1:45:53.0, ICRS 2000.0) of Constellation Virgo, the Earth-Goddess -- northwest of . However, over the thousands of years of astronomy stemming from the Middle East, through the Greeks, Arabs during the Middle Ages, to the Europeans by the Renaissance each star has accumulated many names. Eta Virginis (η Virginis, abbreviated Eta Vir, η Vir) is a triple star system in the zodiac constellation of Virgo.From parallax measurements taken during the Hipparcos mission it is about 265 light-years (81 parsecs) from the Sun.It has a combined apparent visual magnitude of 3.89, bright enough to be seen with the naked eye in dark skies.. Its type is B1 III-IV, so it is intermediate between a giant and sub-giant star. The Variable Type is usually named after the first star of that type to be spotted. Zavijava (Beta Virginis) is a blue to white main sequence star that can be located in the constellation of Virgo. Beta Virginis (β Virginis, viết tắt Beta Vir, β Vir), tên chính thức của nó là Zavijava / ˌ z æ v ɪ ˈ dʒ æ v ə /, (mặc dù nó được chỉ định là ' beta ') là thứ năm - ngôi sao đẹp nhất trong chòm sao Xử Nữ. Zavijava (Beta Virginis), a magnitude 3.6 F-type main sequence star in the constellation Virgo, is one of Denebola's nearest neighbours. Zavijava; edit. At least some of the X-rays are believed to be produced by collisions of the stars' stellar winds. A G-type main-sequence star (Spectral type: G-V), often (and imprecisely) called a yellow dwarf, or G dwarf star, is a main-sequence star (luminosity class V) of spectral type G. Such a star has about 0.84 to 1.15 solar masses and surface temperature of between 5,300 and 6,000 K. [2], Tables VII, VIII. Not Beta Read (1368) Fluff and Angst (1363) Anakin Skywalker Needs a Hug (1332) Include Bookmarker's Tags Star Wars (2380) Star Wars - All Media Types (2169) To Read (2083) Complete (1866) Time Travel (1423) WIP (1053) Clones (948) Series (897) Star Wars: The Clone Wars (2008) - All Media Types (701) Short (635) Other work tags to include Other bookmarker's tags to include Exclude ? Powerplay. Alpha Virginis B is cooler, smaller and less massive, with a temperature of 20,900 K, a radius 3.74 times that of the Sun and a mass of 7.21 solar masses. Beta Lyrae variables are a class of close binary stars.Their total brightness is variable because the two component stars orbit each other, and in this orbit one component periodically passes in front of the other one, thereby blocking its light. Canopus Alpha Carinae 313 ly 2 Yellow-White Supergiant 21. Mimosa Beta Crucis 350 ly 20 . HD66171 0.90 HD240344 19.2 HD124320 2.50 HZ948 1.25 . (See Sloan Digital Sky Survey field images of Zavijava from WikiSky.org.) Controlling system. Hubble's Variable Nebula. Answer (1 of 2): β Tauri or (rarely used) γ Aurigae is commonly known as Elnath, El Nath or Alnath. Beta Virginis (β Vir, β Virginis) is a star in the constellation Virgo.It has the traditional names Zavijava (also Zavijah) and Alaraph. It has reached a stage in its evolution where the hydrogen fuel in its core is exhausted, and thus the star has started to expand, it already has expanded up to more than 10 solar radii. The star is too dim to been seen from Earth with the help of a visual aid. Asset lost on defeat: Tummino's Stockade. Entertainment. Diagram showing how to locate the star Spica using Arcturus as a guide. Gamma Virginis. Spectral classification is based on the strength and width of Balmer hydrogen lines . HR Stars Index. We have used the Sydney University Stellar Interferometer (SUSI) to measure the angular diameter of the F9 V star beta Virginis. Most of these stars are very similar to the Sun and it is probable that there are many Earth-like planets around these stars. This would explain why the observed lower limit of the orbital periods of the binary β Cephei stars is about three times the theoretical lower limit . Spica, also called Alpha Virginis, is a star located in the constellation Virgo, about 10 degrees south of the ecliptic. SIMBAD . Request PDF | Asteroseismology of solar-type stars: Particular physical effects | Since the success of helioseismology, numerous efforts have been made to detect solar-like oscillations on other . That is Arabic for an-nath = the bull's horn (the other horn being ζ Tauri). From these results, it is suggested that the tidal interactions have a damping effect on β Cephei type pulsations. stated in. The star's BD Number is 02 3683.
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