Delta3 Tauri

Star in the constellation Taurus


title: "Delta3 Tauri" type: doc version: 1 created: 2026-02-28 author: "Wikipedia contributors" status: active scope: public tags: ["a-type-subgiants", "am-stars", "binary-stars", "hyades-(star-cluster)", "bayer-objects", "taurus-(constellation)", "stars-with-proper-names", "durchmusterung-objects", "flamsteed-objects", "henry-draper-catalogue-objects", "hipparcos-objects", "bright-star-catalogue-objects", "a-type-main-sequence-stars"] description: "Star in the constellation Taurus" topic_path: "science/astronomy" source: "https://en.wikipedia.org/wiki/Delta3_Tauri" license: "CC BY-SA 4.0" wikipedia_page_id: 0 wikipedia_revision_id: 0

::summary Star in the constellation Taurus ::

| name = δ3 Tauri | image = [[File:HyadesStarMap.jpg|280px]] | caption=Location of δ3 Tauri in the Hyades, indicated by its Flamsteed designation 68 | epoch = J2000.0 | equinox = J2000.0 (ICRS) | constell = Taurus | ra = | dec = | appmag_v = +4.32 (4.35 + 8.37) | class = A2IV-Vs | b-v = | u-b = | variable = | radial_v = | prop_mo_ra = +41.91 | prop_mo_dec = −34.54 | parallax = 21.96 | p_error = 0.51 | parallax_footnote = | absmag_v = +1.14 | source = | mass = | radius = 2.4 | luminosity = 29.5 | temperature = 9,025 | gravity = 3.95 | metal_fe = +0.32 | rotational_velocity = 11.3 | rotation = 2.13 days | age_myr = 630 | names = | Simbad = del03+Tau Delta3 Tauri (δ3 Tauri) is a binary star system in the zodiac constellation of Taurus. Based upon an annual parallax shift of 21.96 mas as seen from Earth, it is located roughly 149 light years distant from the Sun. It is visible to the naked eye with a combined apparent visual magnitude of +4.32. δ3 Tauri is separated from δ1 Tauri by 0.72° on the sky. Some modern astronomy books give this star the name Cleeia, from the Greek Kleeia (transliteration of Κλεεια), who was one of the Hyades sisters. It is considered a member of the Hyades cluster.

In Chinese, 畢宿 (Bì Xiù), meaning Net, refers to an asterism consisting δ3 Tauri, ε Tauri, δ1 Tauri, γ Tauri, Aldebaran, 71 Tauri and λ Tauri. Consequently, the Chinese name for δ3 Tauri itself is 畢宿二 (Bì Xiù èr), "the Second Star of Net".

The magnitude 4.35 primary, component A, appears to be an A-type star intermediate between main sequence and subgiant, with a stellar classification of A2 IV-Vs. The "s" indicates sharp (unusually narrow) absorption lines, a sign of slow rotation. It is a candidate blue straggler and shows characteristics of an Am star. Abt (1985) gave it a classification of A2kA3hA5m, indicating that the spectrum displays the calcium K-line of an A2 star, the hydrogen lines of an A3 star and the metal lines of an A5 star. It is deficient in scandium but has enhanced iron peak and heavy elements. Although suspected of variability in the past, Delta3 Tauri A was subsequently determined to be photometrically constant.

The companion, component B, is a magnitude 8.37 star at an angular separation of 1.80 arc seconds along a position angle of 341°, as of 2010. At 77 arcseconds away (as of 2006) is a magnitude 11.12 visual companion, designated component C.

References

| title=Validation of the new Hipparcos reduction | last1=van Leeuwen | first1=F. | journal=Astronomy and Astrophysics | volume=474 | issue=2 | pages=653–664 | date=2007 | arxiv=0708.1752 | bibcode=2007A&A...474..653V | doi=10.1051/0004-6361:20078357 | s2cid=18759600 | postscript=. }}

| display-authors=1 | last1=Mason | first1=B. D. | last2=Wycoff | first2=G. L. | last3=Hartkopf | first3=W. I. | last4=Douglass | first4=G. G. | last5=Worley | first5=C. E. | journal=The Astronomical Journal | postscript=. | title=The Washington Visual Double Star Catalog | pages=3466–3471 | volume=122 | year=2014 | issue=6 | bibcode=2001AJ....122.3466M | doi=10.1086/323920 | doi-access=free }}

| title=65th Name-List of Variable Stars | display-authors=1 | last1=Kholopov | first1=P. N. | last2=Samus' | first2=N. N. | last3=Kukarkina | first3=N. P. | last4=Medvedeva | first4=G. I. | last5=Perova | first5=N. B. | journal=Information Bulletin on Variable Stars | volume=1921 | page=1 | date=February 1981 | bibcode=1981IBVS.1921....1K | postscript=. }}

| title=On the possible variability of metallic-line and Mercury-Manganese stars | last1=Adelman | first1=S. J. | postscript=. | journal=Astronomy & Astrophysics Supplement Series | volume=123 | date=June 1997 | issue=3 | pages=445–447 | doi=10.1051/aas:1997167 | bibcode=1997A&AS..123..445A | doi-access=free }}

| title=Family of the Hyades | work=Theoi Greek Mythology | url=https://www.theoi.com/Nymphe/NymphaiHyades.html | access-date=2017-08-08 | postscript=. }}

| title=The Mythology of the Night Sky: An Amateur Astronomer's Guide to the Ancient Greek and Roman Legends | series=The Patrick Moore Practical Astronomy Series | first1=David E. | last1=Falkner | postscript=. | publisher=Springer Science & Business Media | year=2011 | isbn=978-1461401377 | page=36 | url=https://books.google.com/books?id=tyj8UUE968wC&pg=PA36 }}

| title=The Star Atlas Companion: What you need to know about the Constellations | series=Springer Praxis Books | first1=Philip M. | last1=Bagnall | publisher=Springer Science & Business Media | year=2012 | isbn=978-1461408307 | page=422 | bibcode=2012sacw.book.....B | url=https://books.google.com/books?id=KcIg02TKW6QC&pg=PA422 }}

| title=Chemical composition of A and F dwarfs members of the Hyades open cluster | last1=Gebran | first1=M. | last2=Vick | first2=M. | last3=Monier | first3=R. | last4=Fossati | first4=L. | journal=Astronomy and Astrophysics | postscript=. | volume=523 | id=A71 | pages=13 | date=November 2010 | doi=10.1051/0004-6361/200913273 | bibcode=2010A&A...523A..71G |arxiv = 1006.5284 | s2cid=7164596 }}

| last1=Eggleton | first1=P. P. | last2=Tokovinin | first2=A. A. | title=A catalogue of multiplicity among bright stellar systems | journal=Monthly Notices of the Royal Astronomical Society | volume=389 | issue=2 | pages=869–879 | date=September 2008 | bibcode=2008MNRAS.389..869E | doi=10.1111/j.1365-2966.2008.13596.x | doi-access=free | arxiv=0806.2878 | s2cid=14878976 | postscript=. }}

| title=The Age Range of Hyades Stars | last1=Eggen | first1=Olin J. | postscript=. | journal=The Astronomical Journal | volume=116 | issue=1 | pages=284–292 | date=July 1998 | doi=10.1086/300413 | bibcode=1998AJ....116..284E | doi-access=free }}

| title=del03 Tau | access-date=2017-08-07 | mode=cs2 | postscript=. }}

References

  1. {{in lang. zh ''中國星座神話'', written by 陳久金. Published by 台灣書房出版有限公司, 2005, {{ISBN. 978-986-7332-25-7.
  2. {{in lang. zh [http://www.lcsd.gov.hk/CE/Museum/Space/Research/StarName/c_research_chinengstars_ala_alz.htm 香港太空館 - 研究資源 - 亮星中英對照表] {{webarchive. link. (2008-10-25 , Hong Kong Space Museum. Accessed on line November 23, 2010.)
  3. (2005). "A catalog of stellar magnetic rotational phase curves". Astronomy and Astrophysics.
  4. (2016). "The Correlation between Metallicity and Debris Disk Mass". The Astrophysical Journal.
  5. (2019). "The Revised TESS Input Catalog and Candidate Target List". The Astronomical Journal.
  6. (1987). "The Early A-Type Stars: Refined MK Classification, Confrontation with Stroemgren Photometry, and the Effects of Rotation". The Astrophysical Journal Supplement Series.
  7. (2014). "The VAST Survey - III. The multiplicity of A-type stars within 75 pc". Monthly Notices of the Royal Astronomical Society.

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a-type-subgiantsam-starsbinary-starshyades-(star-cluster)bayer-objectstaurus-(constellation)stars-with-proper-namesdurchmusterung-objectsflamsteed-objectshenry-draper-catalogue-objectshipparcos-objectsbright-star-catalogue-objectsa-type-main-sequence-stars