Bright white star in #Centaurus, mag 2.73.
🌡️ 9160 K | 2.36 M☉ | 2.1 R☉ | 58 ly
Name Kùlóu (“Arsenal”), from a 2nd-century BCE Chinese super-constellation spanning Centaurus & Lupus.
Shows strong IR excess from a warm debris disk.
#Kulou #IAUStarNames
Bright white star in #Centaurus, mag 2.73.
🌡️ 9160 K | 2.36 M☉ | 2.1 R☉ | 58 ly
Name Kùlóu (“Arsenal”), from a 2nd-century BCE Chinese super-constellation spanning Centaurus & Lupus.
Shows strong IR excess from a warm debris disk.
#Kulou #IAUStarNames
Eruptive Be star in #Cassiopeia, mag 2.4.
🌡️ 26,500 K | 18.7 M☉ | 10.9 R☉ | 549 ly
Name Tiān Sì (“Heavenly Quadriga”), a 2,000-year-old Chinese asterism.
A high-mass X-ray system; X-rays likely from the Be star + disk.
#Tiansi #IAUStarNames
Eruptive Be star in #Cassiopeia, mag 2.4.
🌡️ 26,500 K | 18.7 M☉ | 10.9 R☉ | 549 ly
Name Tiān Sì (“Heavenly Quadriga”), a 2,000-year-old Chinese asterism.
A high-mass X-ray system; X-rays likely from the Be star + disk.
#Tiansi #IAUStarNames
Blue supergiant in #Cassiopeia, mag 4.16.
🌡️ 24,600 K | 38 M☉ | 43 R☉ | 4,126 ly | BC0.7 Ia
Name from Chinese Cè Xīng (“The Whip Star”), part of the charioteer Wangliang.
A fast runaway star with a huge bow shock.
#Cexing #IAUStarNames
Blue supergiant in #Cassiopeia, mag 4.16.
🌡️ 24,600 K | 38 M☉ | 43 R☉ | 4,126 ly | BC0.7 Ia
Name from Chinese Cè Xīng (“The Whip Star”), part of the charioteer Wangliang.
A fast runaway star with a huge bow shock.
#Cexing #IAUStarNames
Orange giant, mag 3.72 in #Auriga.
🌡️ 4,786 K | 1.1 M☉ | 21 R☉ | 140 ly | K0 IIIb
Name from Chinese Bā Gǔ (“Eight Kinds of Crops”), an ancient Han-era asterism.
Brightest star of Bagu & namesake of the Delta Aurigids.
#Bagu #IAUStarNames
Orange giant, mag 3.72 in #Auriga.
🌡️ 4,786 K | 1.1 M☉ | 21 R☉ | 140 ly | K0 IIIb
Name from Chinese Bā Gǔ (“Eight Kinds of Crops”), an ancient Han-era asterism.
Brightest star of Bagu & namesake of the Delta Aurigids.
#Bagu #IAUStarNames
🌡️ 7,680 K | 3.25 M☉ | 3.4 R☉ | 124 ly | A5 III
Name from Arabic al-Aybasān, “the Two Bone-Joints.”
A 31.4-day spectroscopic binary as tight as Mercury’s orbit.
#Alaybasan #IAUStarNames #BinaryStars
🌡️ 7,680 K | 3.25 M☉ | 3.4 R☉ | 124 ly | A5 III
Name from Arabic al-Aybasān, “the Two Bone-Joints.”
A 31.4-day spectroscopic binary as tight as Mercury’s orbit.
#Alaybasan #IAUStarNames #BinaryStars
🌡️ 9,440 K | 2.5 M☉ | 2.25 R☉ | 117 ly | A1Vnn
From ancient Egyptian Apdu (𓅫pd), “the Bird,” now official IAU name.
#Apdu #GammaTrianguli #IAUStarNames #StarEtymology #Triangulum
🌡️ 9,440 K | 2.5 M☉ | 2.25 R☉ | 117 ly | A1Vnn
From ancient Egyptian Apdu (𓅫pd), “the Bird,” now official IAU name.
#Apdu #GammaTrianguli #IAUStarNames #StarEtymology #Triangulum
🌡️ 4,840 K | 2.5 M☉ | 10 R☉ | 195 ly | K0 IIIb
From Arabic al-dhayl, “the hem (of a robe),” marking the lower hem of Andromeda’s dress.
#Adhil #IAUStarNames #ArabicAstronomy #RedGiant
🌡️ 4,840 K | 2.5 M☉ | 10 R☉ | 195 ly | K0 IIIb
From Arabic al-dhayl, “the hem (of a robe),” marking the lower hem of Andromeda’s dress.
#Adhil #IAUStarNames #ArabicAstronomy #RedGiant
🌡️ 3,460 K | 6.5 M☉ | 101 R☉ | 1,770 ly | K1 II
From Arabic ʿAyn ar-Rāmī, “the Eye of the Archer.”
#Ainalrami #IAUStarNames #ArabicAstronomy #Supergiant
🌡️ 3,460 K | 6.5 M☉ | 101 R☉ | 1,770 ly | K1 II
From Arabic ʿAyn ar-Rāmī, “the Eye of the Archer.”
#Ainalrami #IAUStarNames #ArabicAstronomy #Supergiant
🌡️ 3,900 K | 1.16 M☉ | 45 R☉ | 65 ly | K5+III
From Arabic al-dabarān, “the Follower,” trailing the Pleiades.
Once Sun-like, now a red giant.
#Aldebaran #ArabicAstronomy #IAUStarNames #RedGiant
🌡️ 3,900 K | 1.16 M☉ | 45 R☉ | 65 ly | K5+III
From Arabic al-dabarān, “the Follower,” trailing the Pleiades.
Once Sun-like, now a red giant.
#Aldebaran #ArabicAstronomy #IAUStarNames #RedGiant
🌡️ 17,360 K | 10 M☉ | 4.3 R☉ | B6 type
Name from Arabic al-aẓfār, “the talons (of the eagle).”
Part of the ancient Arabian Eagle asterism.
#IAUStarNames #ArabicAstronomy #BlueStar #Lyra
🌡️ 17,360 K | 10 M☉ | 4.3 R☉ | B6 type
Name from Arabic al-aẓfār, “the talons (of the eagle).”
Part of the ancient Arabian Eagle asterism.
#IAUStarNames #ArabicAstronomy #BlueStar #Lyra
🌡️ 4,880 K | 2.45 M☉ | 12 R☉
Hosts giant planet Amateru (ε Tau b), a hot super-Jupiter (~7 M♃) orbiting every 586 d.
Name “Ain” = Arabic ʿAyn al-Thawr, “Bull’s Eye.”
#Ain #Amateru #IAUStarNames #Exoplanet #Taurus
🌡️ 4,880 K | 2.45 M☉ | 12 R☉
Hosts giant planet Amateru (ε Tau b), a hot super-Jupiter (~7 M♃) orbiting every 586 d.
Name “Ain” = Arabic ʿAyn al-Thawr, “Bull’s Eye.”
#Ain #Amateru #IAUStarNames #Exoplanet #Taurus
A white giant star in Scorpius, once known in Chinese uranography as the Divine Palace, part of the Tail of the Azure Dragon.
Its soft Milky Way glow was seen as a sacred hall among the stars.
IAU-Adopted(2025).
#Shengong #ChineseAstronomy #WGSN #CulturalAstronomy
A white giant star in Scorpius, once known in Chinese uranography as the Divine Palace, part of the Tail of the Azure Dragon.
Its soft Milky Way glow was seen as a sacred hall among the stars.
IAU-Adopted(2025).
#Shengong #ChineseAstronomy #WGSN #CulturalAstronomy
IAU releases the ancient Sanskrit name “Apāmvatsa,” meaning “calf of the waters,” from Indian sky tradition — just in time for Deepavali’s lights and Halloween’s pumpkins.
🌡️ 3,500 K | 400 ly | M2.5 III
#Apamvatsa #IAUStarNames
IAU releases the ancient Sanskrit name “Apāmvatsa,” meaning “calf of the waters,” from Indian sky tradition — just in time for Deepavali’s lights and Halloween’s pumpkins.
🌡️ 3,500 K | 400 ly | M2.5 III
#Apamvatsa #IAUStarNames
He showed how ancient Iberian sites — from Antequera Dolmens to Talayotic Menorca — reveal humanity’s timeless bond with the sky.
#IAU #StarNames
He showed how ancient Iberian sites — from Antequera Dolmens to Talayotic Menorca — reveal humanity’s timeless bond with the sky.
#IAU #StarNames
#IAU #WGSN #Astronomy
#IAU #WGSN #Astronomy
Faint companion of #Betelgeuse in Orion, mag ~8.2. Predicted long ago, revealed by speckle imaging in 2020 & 2024.
🌡️ ~7,400 K | ~1.6 M☉ | ~1.5 R☉ | 548 ly
🔬 Likely F-type
Name “Siwarhā” = “her bracelet,” from Arabic lore of al-Jawzāʼ.
#Siwarha
Faint companion of #Betelgeuse in Orion, mag ~8.2. Predicted long ago, revealed by speckle imaging in 2020 & 2024.
🌡️ ~7,400 K | ~1.6 M☉ | ~1.5 R☉ | 548 ly
🔬 Likely F-type
Name “Siwarhā” = “her bracelet,” from Arabic lore of al-Jawzāʼ.
#Siwarha
A blue-white subgiant (mag 4.48) in Cetus and 3rd-brightest member of the Psc–Eri stellar stream (~4,700 stars).
🌡️ 11,419 K | 2.68 M☉ | 2.75 R☉ | 272 ly
🔬 B9 IVn
Greek name ὕδωρ “Water,” once misplaced in Aquarius, restored by IAU in 2019.
#Hydor #Cetus
A recurrent nova in the Northern Crown, normally mag ~10 but erupting every ~80 yrs to naked-eye brightness (mag 2).
🌡️ 3,561 K | ~0.93 M☉ | ~63 R☉ | ~2,990 ly
💫 Symbiotic binary: red giant + white dwarf.
Historic eruptions in 1866 & 1946.
#BlazeStar #Nova
A recurrent nova in the Northern Crown, normally mag ~10 but erupting every ~80 yrs to naked-eye brightness (mag 2).
🌡️ 3,561 K | ~0.93 M☉ | ~63 R☉ | ~2,990 ly
💫 Symbiotic binary: red giant + white dwarf.
Historic eruptions in 1866 & 1946.
#BlazeStar #Nova
A red giant glowing at mag 3.8 in Aquarius, ~391 ly away.
🌡️ 3,702 K | 2.96 M☉ | 100 R☉ | M2.5III
📜 Sanskrit “Shatabhisha” (शतभिषज्) = “hundred physicians,” a Vedic name >3,000 yrs old, later reimagined as hundred stars.
💫 Companion star detected.
✅ Adopted by IAU.
A red giant glowing at mag 3.8 in Aquarius, ~391 ly away.
🌡️ 3,702 K | 2.96 M☉ | 100 R☉ | M2.5III
📜 Sanskrit “Shatabhisha” (शतभिषज्) = “hundred physicians,” a Vedic name >3,000 yrs old, later reimagined as hundred stars.
💫 Companion star detected.
✅ Adopted by IAU.
Hot B-type binary in Andromeda, mag 4.5, 720 ly.
🌡️ ~13,490 K | 7.6 M☉ | 5.5 R☉ | B7 Ve
💫 Wide binary, ~554 yr orbit, rapid rotation.
📜 Name = “Southern Military Gate” (軍南門) in Chinese tradition.
✅ IAU-adopted Aug 2025
#Junnanmen #IAU
Hot B-type binary in Andromeda, mag 4.5, 720 ly.
🌡️ ~13,490 K | 7.6 M☉ | 5.5 R☉ | B7 Ve
💫 Wide binary, ~554 yr orbit, rapid rotation.
📜 Name = “Southern Military Gate” (軍南門) in Chinese tradition.
✅ IAU-adopted Aug 2025
#Junnanmen #IAU
Hot B-type star in Perseus ♢ mag 4.06 from 720 ly
🌡️ ~29,300 K | 9.6 M☉ | 5.5 R☉ | B2Vep
💫 Runaway O/B-type binary w/ circumstellar disk
📜 Named “Heaven’s Great General” in Chinese asterism Dajiangjun
✅ Adopted by IAU in Aug 2025
#Dajiangjunbei #StarNames
Hot B-type star in Perseus ♢ mag 4.06 from 720 ly
🌡️ ~29,300 K | 9.6 M☉ | 5.5 R☉ | B2Vep
💫 Runaway O/B-type binary w/ circumstellar disk
📜 Named “Heaven’s Great General” in Chinese asterism Dajiangjun
✅ Adopted by IAU in Aug 2025
#Dajiangjunbei #StarNames
Close binary in Triangulum ♢, shining at mag 5.3 from 289 ly away.
🌡️ ~4,930 K | 2.5 M☉ | 4 R☉ | G0 III
💫 RS CVn-type with starspots & ellipsoidal variability.
📜 Name from Hevelius’s Triangulum Minus asterism.
✅ Adopted by IAU in Aug 2025.
#Triminus #StarNames
Close binary in Triangulum ♢, shining at mag 5.3 from 289 ly away.
🌡️ ~4,930 K | 2.5 M☉ | 4 R☉ | G0 III
💫 RS CVn-type with starspots & ellipsoidal variability.
📜 Name from Hevelius’s Triangulum Minus asterism.
✅ Adopted by IAU in Aug 2025.
#Triminus #StarNames
WGSN adopts star names from Chinese & ancient Greek traditions — highlighting asterisms in Andromeda, Perseus, Cetus & Triangulum, from classical astronomy to early modern heritage.
Names now in the IAU Star Names Catalog 🔗 exopla.net/star-names
#WGSN #IAU #StarNames
WGSN adopts star names from Chinese & ancient Greek traditions — highlighting asterisms in Andromeda, Perseus, Cetus & Triangulum, from classical astronomy to early modern heritage.
Names now in the IAU Star Names Catalog 🔗 exopla.net/star-names
#WGSN #IAU #StarNames
The brightest star of Crux, the Southern Cross 🌌 mag 0.76, 321 ly.
Spectral type B0.5IV: 🌡️ 28,800 K | 17 M☉ | 7 R☉
Visible south of the Tropic of Cancer, Acrux has long guided navigation.
✅ Officially adopted by the IAU.
#Acrux #Crux #IAUStarNames
The brightest star of Crux, the Southern Cross 🌌 mag 0.76, 321 ly.
Spectral type B0.5IV: 🌡️ 28,800 K | 17 M☉ | 7 R☉
Visible south of the Tropic of Cancer, Acrux has long guided navigation.
✅ Officially adopted by the IAU.
#Acrux #Crux #IAUStarNames