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Supernova observed from Earth in 1006
SN 1006 was a supernova that is likely the brightest observed stellar event in recorded history, reaching an estimated −7.5 visual magnitude, and exceeding
SN_1006
Calendar year
Hindu Mataram kingdom. April 30 – The brightest supernova ever recorded, SN 1006, occurs in the constellation of Lupus. It is observed and described in
1006
Supernova in the constellation Taurus; visible from 1054 to 1056
written accounts which precede the invention of the telescope (SN 1006, SN 1181, SN 1572 and SN 1604) are however established with reasonable certitude. Telescope-era
SN_1054
Astrophysical phenomenon
prehistoric people. The first widely recorded supernova was SN 1006, observed in AD 1006 in the constellation of Lupus. This event was described by observers
Supernova
Egyptian astrologer and astronomer
of the supernova now known as SN 1006, the brightest stellar event in recorded history, which he observed in the year 1006. This was written in a commentary
Ali_ibn_Ridwan
Type of supernova in binary systems
white dwarf have been ruled out. It has also been strongly suggested for SN 1006, given that no companion star remnant has been found there. Observations
Type_Ia_supernova
Possible supernova in 393 AD and it is in Scorpius
SN 393 is the modern designation for a probable supernova that was reported by the Chinese in the year 393 CE. An extracted record of this astronomical
SN_393
ISSN 0035-8711. Winkler, P. Frank; Gupta, Gaurav; Long, Knox S. (2003). "The SN 1006 Remnant: Optical Proper Motions, Deep Imaging, Distance, and Brightness
List of supernovae (before 2000)
List_of_supernovae_(before_2000)
Ancient and modern recorded observations of supernovae explosions
Indian and other observers. The supernova SN 1006 appeared in the southern constellation of Lupus during the year 1006 CE. This was the brightest recorded star
History of supernova observation
History_of_supernova_observation
Astronomy in Ancient Egypt
observations on eclipses were still used centuries later. In 1006, Ali ibn Ridwan observed the SN 1006, a supernova regarded as the brightest stellar event in
Egyptian_astronomy
Red supergiant star in the constellation Orion
Models of rotating 20 M☉ stars predict a peculiar Type II supernova similar to SN 1987A from a blue supergiant progenitor. On the other hand, non-rotating 20 M☉
Betelgeuse
Constellation in the southern celestial hemisphere
constellation. The historic supernova SN 1006 is described by various sources as appearing on April 30 to May 1, 1006, in the constellation of Lupus. ESO
Lupus_(constellation)
Scientific study of celestial objects
Muslim astronomer Abd al-Rahman al-Sufi in his Book of Fixed Stars. The SN 1006 supernova, the brightest apparent magnitude stellar event in the last 1000
Astronomy
Stellar core remnant
instabilities that could create a neutron star. The historical bright SN 1006 is thought to have been a Type Ia supernova from a white dwarf, possibly
White_dwarf
Brighter component of a wide double star system in the constellation Lupus
clusters NGC 5749 NGC 5822 NGC 5824 NGC 5927 NGC 5986 Nebulae IC 4406 NGC 5882 Galaxies IC 4444 NGC 5530 NGC 5643 Astronomical events SN 1006 Category
Zeta_Lupi
Chronological list of developments in knowledge and records
astronomers become the first to record observations of a supernova, SN 185. 1006 – SN 1006, a magnitude −7.5 supernova in the constellation of Lupus, is observed
Timeline of white dwarfs, neutron stars, and supernovae
Timeline_of_white_dwarfs,_neutron_stars,_and_supernovae
Sudden release of heat and gas
Hunga-Ha'apai eruption Oruanui eruption Toba supereruption Yellowstone Caldera SN 1006 SN 1572 Kepler's Supernova Solar storm of 1859 Meteor Crater Chichxulub impact
Explosion
Remnants of an exploded star
needed to generate ultra-high-energy cosmic rays. Observations of the SN 1006 remnant in X-rays have shown synchrotron emission consistent with it being
Supernova_remnant
Binary star in the constellation Lupus
clusters NGC 5749 NGC 5822 NGC 5824 NGC 5927 NGC 5986 Nebulae IC 4406 NGC 5882 Galaxies IC 4444 NGC 5530 NGC 5643 Astronomical events SN 1006 Category
Kappa_Lupi
26,000 Ib or Ic Milky Way unidentified black hole SN 1006 15h 02m 22.1s −42° 05′ 49″ May 1, 1006 −7.5 7,200 Ia Milky Way none G350.1-0.3 17h 21m 06s
List_of_supernova_remnants
Coming together of two stars
September 2012). "No surviving evolved companions of the progenitor of SN 1006". Nature. 489 (7417): 533–536. arXiv:1210.1948. Bibcode:2012Natur.489.
Stellar_collision
Triple star system in the constellation Lupus
clusters NGC 5749 NGC 5822 NGC 5824 NGC 5927 NGC 5986 Nebulae IC 4406 NGC 5882 Galaxies IC 4444 NGC 5530 NGC 5643 Astronomical events SN 1006 Category
Xi_Lupi
Hydrogen gas region in outer space approximately 100 AU in size
Knots or globules of denser gas in SN 1006.
Evaporating_gaseous_globule
as a collection of numerous nebulous stars 1006 — Ali ibn Ridwan and Chinese astronomers observe the SN 1006, the brightest stellar event ever recorded
Timeline_of_stellar_astronomy
Large self-illuminated object in space
supernova, now known as SN 185. The brightest stellar event in recorded history was the SN 1006 supernova, which was observed in 1006 and written about by
Star
Probable triple star system in the constellation of Lupus
clusters NGC 5749 NGC 5822 NGC 5824 NGC 5927 NGC 5986 Nebulae IC 4406 NGC 5882 Galaxies IC 4444 NGC 5530 NGC 5643 Astronomical events SN 1006 Category
Eta_Lupi
Brightness of a celestial object observed from the Earth
December 2011. Winkler, P. Frank; Gupta, Gaurav; Long, Knox S. (2003). "The SN 1006 Remnant: Optical Proper Motions, Deep Imaging, Distance, and Brightness
Apparent_magnitude
Star in the constellation Lupus
clusters NGC 5749 NGC 5822 NGC 5824 NGC 5927 NGC 5986 Nebulae IC 4406 NGC 5882 Galaxies IC 4444 NGC 5530 NGC 5643 Astronomical events SN 1006 Category
Tau1_Lupi
Systematic designations to unambiguously identify astronomical objects
they occurred: SN 1006 (the brightest stellar event ever recorded), SN 1054 (of which the remnant is the Crab Nebula and the Crab Pulsar), SN 1572 (Tycho's
Astronomical naming conventions
Astronomical_naming_conventions
Stellar system in the constellation Carina
brighter, potentially the brightest supernova in recorded history (currently SN 1006). At 7,500 light-years from the star it is unlikely to directly affect
Eta_Carinae
Overview of the scientific field of astronomy
Supernovae in fiction SN 1054 Supergiant Crab Nebula Tycho's Kepler's SN 1987A SN 185 SN 1006 SN 2003fg Vela Supernova Remnant Remnant G1.9+0.3 SN 2007bi Research
Outline_of_astronomy
the Large Magellanic Cloud was also given by al-Sufi. In 1006, Ali ibn Ridwan observed SN 1006, the brightest supernova in recorded history, and left a
History_of_astronomy
Star in the constellation Lupus
clusters NGC 5749 NGC 5822 NGC 5824 NGC 5927 NGC 5986 Nebulae IC 4406 NGC 5882 Galaxies IC 4444 NGC 5530 NGC 5643 Astronomical events SN 1006 Category
Phi1_Lupi
Logarithmic measure of the brightness of an astronomical object
50×10−14 near-infrared light limit of James Webb Space Telescope −7 631 SN 1006 supernova 14 2.51×10−6 Pluto (max.) limit of 8–10 in (20–25 cm) telescopes
Magnitude_(astronomy)
L'Anse aux Meadows 1006 SN 1006 supernova, brightest apparent magnitude stellar event in recorded history (−7.5 visual magnitude) 1054 SN 1054 supernova,
Timeline of environmental history
Timeline_of_environmental_history
Supernova remnant in the constellation Gemini
radio morphology is shell-like (e.g. a prototypical shell-like SNR is SN 1006), consisting of two connected sub-shells with different centers and radii
IC_443
the SN 185, recorded during the Han dynasty. Chinese astronomers made two more notable supernova observations during the Song dynasty: the SN 1006, the
History of science and technology in China
History_of_science_and_technology_in_China
American space scientist
Observation of the Nonradiative Collisionless Shock in the Remnant of SN 1006". The Astrophysical Journal. 615 (1): 280–285. Bibcode:2004ApJ...615..280K
Kelly_Korreck
Earth UDF 2457 m= 25 Brightest star in a transient event Progenitor of SN 1006 1006 m= −7.5 This was a supernova, and its remnant (SNR) is catalogued as
List_of_star_extremes
B-type main-sequence star
clusters NGC 5749 NGC 5822 NGC 5824 NGC 5927 NGC 5986 Nebulae IC 4406 NGC 5882 Galaxies IC 4444 NGC 5530 NGC 5643 Astronomical events SN 1006 Category
Sigma_Lupi
Binary star system in the constellation Lupus
clusters NGC 5749 NGC 5822 NGC 5824 NGC 5927 NGC 5986 Nebulae IC 4406 NGC 5882 Galaxies IC 4444 NGC 5530 NGC 5643 Astronomical events SN 1006 Category
Tau2_Lupi
Star in the constellation Lupus
clusters NGC 5749 NGC 5822 NGC 5824 NGC 5927 NGC 5986 Nebulae IC 4406 NGC 5882 Galaxies IC 4444 NGC 5530 NGC 5643 Astronomical events SN 1006 Category
Upsilon_Lupi
years ago. The Schweizer–Middleditch Star is a star near the center of SN 1006 in Centaurus. Named after Francois Schweizer and John Middleditch. Sneden's
Stars_named_after_people
Star in the constellation Lupus
clusters NGC 5749 NGC 5822 NGC 5824 NGC 5927 NGC 5986 Nebulae IC 4406 NGC 5882 Galaxies IC 4444 NGC 5530 NGC 5643 Astronomical events SN 1006 Category
Nu1_Lupi
Binary star system in the constellation Lupus
clusters NGC 5749 NGC 5822 NGC 5824 NGC 5927 NGC 5986 Nebulae IC 4406 NGC 5882 Galaxies IC 4444 NGC 5530 NGC 5643 Astronomical events SN 1006 Category
Omicron_Lupi
Star in the constellation Lupus
clusters NGC 5749 NGC 5822 NGC 5824 NGC 5927 NGC 5986 Nebulae IC 4406 NGC 5882 Galaxies IC 4444 NGC 5530 NGC 5643 Astronomical events SN 1006 Category
Rho_Lupi
Japanese cosmic X-ray astronomy mission
X-ray image of SN 1006, taken by ASCA
Advanced Satellite for Cosmology and Astrophysics
Advanced_Satellite_for_Cosmology_and_Astrophysics
Star in the constellation Lupus
clusters NGC 5749 NGC 5822 NGC 5824 NGC 5927 NGC 5986 Nebulae IC 4406 NGC 5882 Galaxies IC 4444 NGC 5530 NGC 5643 Astronomical events SN 1006 Category
Omega_Lupi
Decade
Hindu Mataram kingdom. April 30 – The brightest supernova ever recorded, SN 1006, occurs in the constellation of Lupus. It is observed and described in
1000s_(decade)
Triple star system in the constellation Lupus
clusters NGC 5749 NGC 5822 NGC 5824 NGC 5927 NGC 5986 Nebulae IC 4406 NGC 5882 Galaxies IC 4444 NGC 5530 NGC 5643 Astronomical events SN 1006 Category
Lambda_Lupi
Italian independent record labels
Frank Tafuri, on "Black Saint/Soul Note: Critics' Pick Sampler" (Vol. 1) BS/SN-C001 Search results for "Black Saint/Soul Note" Archived 2014-10-08 at the
Black_Saint/Soul_Note
Star in the constellation of Lupus
transverse velocity. It is positioned about 1.3° SSW of the supernova remnant SN 1006. In Chinese, 騎官 (Qí Guān), meaning Imperial Guards, refers to an asterism
Beta_Lupi
Star in the constellation Lupus
clusters NGC 5749 NGC 5822 NGC 5824 NGC 5927 NGC 5986 Nebulae IC 4406 NGC 5882 Galaxies IC 4444 NGC 5530 NGC 5643 Astronomical events SN 1006 Category
Iota_Lupi
Star in the constellation Lupus
clusters NGC 5749 NGC 5822 NGC 5824 NGC 5927 NGC 5986 Nebulae IC 4406 NGC 5882 Galaxies IC 4444 NGC 5530 NGC 5643 Astronomical events SN 1006 Category
Theta_Lupi
11th-century Arab Christian physician from Baghdad
art' when he described the supernova SN 1006. This supernova was witnessed by Ibn Riḍwān in April and May 1006 AD/Raǧab of 396 AH, termed by him to have
Ibn_Butlan
Laboratory SLOWPOKE reactor SMART-1 SNO+ SNOLAB SNUPPS SN 1006 SN 1987A SN 2002cx SN 2003fg SN 2005gj SN 2007bi SO(10) (physics) SOFAR channel SOLEIL SPEAR
Index_of_physics_articles_(S)
distance for the brightest supernova event recorded in human history, SN 1006, as being ~7,200 light years distant. Winkler has received multiple U.S
Frank_Winkler
Multiple star system in the constellation of Lupus
clusters NGC 5749 NGC 5822 NGC 5824 NGC 5927 NGC 5986 Nebulae IC 4406 NGC 5882 Galaxies IC 4444 NGC 5530 NGC 5643 Astronomical events SN 1006 Category
Mu_Lupi
Star in the constellation Lupus
clusters NGC 5749 NGC 5822 NGC 5824 NGC 5927 NGC 5986 Nebulae IC 4406 NGC 5882 Galaxies IC 4444 NGC 5530 NGC 5643 Astronomical events SN 1006 Category
Phi2_Lupi
Star in the constellation Lupus
clusters NGC 5749 NGC 5822 NGC 5824 NGC 5927 NGC 5986 Nebulae IC 4406 NGC 5882 Galaxies IC 4444 NGC 5530 NGC 5643 Astronomical events SN 1006 Category
Psi2_Lupi
Chemical compound
In the gas phase SnBr2 is non-linear with a bent configuration similar to SnCl2 in the gas phase. The Br-Sn-Br angle is 95° and the Sn-Br bond length is
Tin(II)_bromide
Chemical compound
(2010). "THERMOPOWER OF SnTe FROM BOLTZMANN TRANSPORT CALCULATIONS". Functional Materials Letters. 03 (4): 223–226. arXiv:1006.4151. doi:10.1142/S1793604710001299
Tin_telluride
American mathematician
Prescribing scalar curvature on Sn and related problems. I. J. Differential Equations 120 (1995), no. 2, 319–410. doi:10.1006/jdeq.1995.1115 Yan Yan Li. Prescribing
YanYan_Li
Class of lipid compounds
Martin A, Wakelam MJ (March 1997). "Purification and characterization of sn-1-stearoyl-2-arachidonoylglycerol kinase from pig testes". Biochem. J. 322
Phosphatidic_acid
Protein-coding gene in the species Homo sapiens
snRNP70 also known as U1 small nuclear ribonucleoprotein 70 kDa is a protein that in humans is encoded by the SNRNP70 gene. snRNP70 is a small nuclear
SnRNP70
Concept in Buddhism
as in: SN 45.179 and 45.180; SN 46.129 and 46.130; SN 46.183 and 46.184; SN 47.103 and 47.104; SN 48.123 and 48.124; SN 49.53 and 49.54; SN 50.53 and
Fetter_(Buddhism)
Fundamental elements in Indian philosophy
Sutta (SN 35.204 or 35.245) Dutiya-mittāmacca Sutta (SN 55.17) Various brief Saṁyutta Nikāya discourses entitled, "Dhātu Sutta" (SN 18.9, SN 25.9, SN 26.9
Mahābhūta
enzyme with systematic name sn-glycerol 3-phosphate:quinone oxidoreductase. This enzyme catalyses the following chemical reaction sn glycerol 3-phosphate +
Glycerol-3-phosphate dehydrogenase (quinone)
Glycerol-3-phosphate_dehydrogenase_(quinone)
Chemical compound
Z)-octadec-9-enoyl]oxy}propyl dihydrogen phosphate Other names LPA 1-acyl-sn-glycerol 3-phosphate Identifiers CAS Number 22002-87-5 Y 3D model (JSmol)
Lysophosphatidic_acid
Galaxy in the constellation Triangulum
being viewed nearly edge on. One supernovae have been observed in NGC 634: SN 2006Q (Type II, mag. 17.2) was discovered by the Lick Observatory Supernova
NGC_634
Hopf algebra with a basis of all elements of all the finite symmetric groups Sn, and is a non-commutative analogue of the Hopf algebra of symmetric functions
Hopf_algebra_of_permutations
Prominent bulge of the occipital bone at the back of the skull
protuberance Terms for anatomical location Varghese E, Samson RS, Kumbargere SN, Pothen M (May 2017). "Occipital spur: understanding a normal yet symptomatic
Occipital_bun
Spiral galaxy in the constellation Ursa Major
Only one supernova has been detected in Messier 81. The supernova, named SN 1993J, was discovered on 28 March 1993 by F. García in Spain. At the time
Messier_81
Area of mathematics
(1996-02-15). "On the Kronecker Product of Sn Characters". Journal of Algebra. 154: 125–140. doi:10.1006/jabr.1993.1008. Littlewood, D. E. (1958). "Products
Representation theory of the symmetric group
Representation_theory_of_the_symmetric_group
Subclass of glycerophospholipids
class of glycerophospholipid with a plasmenyl group linked to a lipid at the sn-1 position of the glycerol backbone. Plasmalogens are found in multiple domains
Plasmalogen
Disorder of decreased tolerance to specific sounds
[Data Collection]. Colchester, Essex: UK Data Service. doi:10.5255/UKDA-SN-856149. Vitoratou S, Hayes C, Uglik-Marucha N, Pearson O, Graham T, Gregory
Misophonia
Protein found in humans
Medicine. 2 (5): 439–44. doi:10.2174/1566524023362311. PMID 12125809. Phillips SN, Benedict JW, Weimer JM, Pearce DA (March 2005). "CLN3, the protein associated
Battenin
Pain in the false ribs due to the partial dislocation of the costal cartilage
"Painful rib syndrome--a review of 76 cases". Gut. 34 (7): 1006–8. doi:10.1136/gut.34.7.1006. ISSN 0017-5749. PMC 1374244. PMID 8344569. McMahon LE (June
Slipping_rib_syndrome
Tabular arrangement of the chemical elements
; Abdullin, F.Sh.; Bailey, P.D.; Benker, D.E.; Bennett, M.E.; Dmitriev, S.N.; et al. (2010). "Synthesis of a new element with atomic number Z = 117"
Periodic_table
Conjecture on zeros of the zeta function
Landau's function given by the maximal order of elements of the symmetric group Sn of degree n, then Massias, Nicolas & Robin (1988) showed that the Riemann
Riemann_hypothesis
Mammalian hormone released from the pituitary gland
PMID 9989497. S2CID 6916996. Wang XM, Dayanithi G, Lemos JR, Nordmann JJ, Treistman SN (November 1991). "Calcium currents and peptide release from neurohypophysial
Vasopressin
RNA family
nuclear RNAs (snRNAs). This type of modifying RNA is usually located in the nucleolus of the eukaryotic cell which is a major site of snRNA biogenesis
Small_nucleolar_RNA_R20
Non-coding RNA component of the spliceosome
snRNP, involved with the U6 snRNA in the di-snRNP, as well as involved with both the U6 snRNA and the U5 snRNA in the tri-snRNP. The different formats have
U4_spliceosomal_RNA
2002–2003 Supernova in the constellation Canis Major
SN 2003H was a supernova that appeared halfway between the colliding NGC 2207 and IC 2163 galaxies. It was discovered on January 8, 2003, by the Lick Observatory
SN_2003H
Chemical compound
3171/jns.1996.84.4.0690. PMID 8613866. S2CID 1172874. Bunawan H, Bunawan SN, Baharum SN, Noor NM (2015). "Sauropus androgynus (L.) Merr. Induced Bronchiolitis
Papaverine
and 40-kDa forms". Genomics. 52 (3): 267–277. doi:10.1006/geno.1998.5443. PMID 9790745. Sarkar SN, Ghosh A, Wang HW, Sung SS, Sen GC (September 1999).
OAS1
American astrophysicist (born 1958)
"Optical light curves of the Type IA supernovae SN 1990N and 1991T". Astronomical Journal 116: 1006. doi:10.1086/300175. Scoville, N. et al. (2007).
Neil_deGrasse_Tyson
Measure of variation in statistics
which the sample is drawn may be much larger). This estimator, denoted by sN, is known as the uncorrected sample standard deviation, or sometimes the standard
Standard_deviation
Lattice formed by all integer partitions
restriction from Sn+1 to Sn is multiplicity-free, and the representation of Sn with partition p is contained in the representation of Sn+1 with partition
Young's_lattice
Type of material
Archaeological Science. 29 (12): 1451–1460. Bibcode:2002JArSc..29.1451T. doi:10.1006/jasc.2002.0809. Kaufman, Brett. "Metallurgy and Archaeological Change in
Metal
Domain of organisms
archaeal phospholipids are built on a backbone of sn-glycerol-1-phosphate, which is an enantiomer of sn-glycerol-3-phosphate, the phospholipid backbone
Archaea
Degenerative disease that affects sheep and goats
Denaturing Gradient Gel Electrophoresis". Genomics. 15 (1): 30–37. doi:10.1006/geno.1993.1006. ISSN 0888-7543. PMID 8094373. CABI (2022-01-07). "scrapie". CABI
Scrapie
Anticonvulsant medication
"Chapter 28 - Herpes Zoster and Postherpetic Neuralgia". In Benzon HT, Raja SN, Liu SS, Fishman SM (eds.). Essentials of Pain Medicine (Fourth ed.). Elsevier
Pregabalin
Municipality in Košice Region, Slovakia
It has a population of 1007 people (31 December 2025). In year 2021 was 1006 people by ethnicity 882 as Slovak, 283 as Rusyn, 255 as Romani, 75 as Not
Poráč
Grouping of stars by similar metallicity
stars Peekaboo Galaxy It has been proposed that recent supernovae SN 2006gy and SN 2007bi may have been pair-instability supernovae where such super-massive
Stellar_population
Time when menstrual periods stop permanently
Kalantaridou SN, Davis SR, Nelson LM (December 1998). "Premature ovarian failure". Endocrinology and Metabolism Clinics of North America. 27 (4): 989–1006. doi:10
Menopause
Manuscripts of the Septuagint translation
century Ps.Od. EBE, 3 Athens Greece 1005 12th century Ps. EBE, 5 Athens Greece 1006 12th century Ps.Od. EBE, 6 Athens Greece 1007 10th/11th century Ps.Od. EBE
Septuagint_manuscripts
Spiral galaxy in the constellation Leo Minor
burned into Hanny's Voorwerp. One supernova has been observed in IC 2497: SN 2020ilb (type Ia, mag. 19) was discovered on 29 April 2020. "IC 2497". SIMBAD
IC_2497
Buddhist term
Piyadassi, Thera (1999). "Gilana Sutta: Ill (Factors of Enlightenment)" (SN 46.14). Retrieved 7 February 2011 from "Access to Insight". Rhys Davids, T
Vīrya
Pathology protocol to assess cancer risk
Oncology. 77 (2): 319–320. doi:10.1006/gyno.2000.5740. ISSN 0090-8258. PMID 10785486. Paley PJ, Swisher EM, Garcia RL, Agoff SN, Greer BE, Peters KL, et al
SEE-FIM_Protocol
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