The yuga of Sphujiddhvaja and the Era of the Kusanas
2001, Silk Road Art and Archaeology
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Abstract
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The paper examines the historical context and significance of the yuga of Sphujiddhvaja in relation to the era of the Kushanas. It discusses the succession and dating of early Kushana kings, focusing on inscriptions that indicate the era initiated by Kaniska. The analysis includes the implications of astronomical knowledge transfer from Western contexts to South Asia, particularly around the establishment of the Saka era and its lasting impact. The findings suggest that the establishment of astronomical systems by Western astronomers in India during the early years of Gondophares' rule had profound cultural implications.
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2025
A first Sothic date for the early 4th dynasty of Egypt seems to be included in the papyrus archive from Wadi el-Jarf. The date would imply that king Khufu accessed the throne between -2603 and -2599 which is fully compliant with modern radiocarbon dates for dynastic Egypt.
Chinese Cultural Relics, 2016
solute dating and cross-dating, the last of which is the combined use of the two preceding types of dating, have been a part of archaeological chronology. Thus far, apart from such minute improvements as the calibration of radiocarbon dates with dendrochronology and the introduction of AMS dating, little progress has been made in these two types of dating compared to the rapid development of many other methods of research in archaeology. If another revolution in archaeology is to be hoped for, it is imperative to advance methods of archaeological dating that cater to the growing needs of archaeology, since even under the current system of archaeological chronology, there are topics that need to be further addressed. By way of illustration, this article elaborates on four of these topics.
--वसुदेवसुतं देवं कंस चाणूर मर्दनम् । A breath-taking moment of divine manifestation detailed in MBh with jyotiṣa pramāṇa. --rationale for the next Kali Era 3102 BCE; to underscore the importance of ethical behaviour by sovereign rulers, kings. --Why was the Saptarṣi maṇḍala, an era which started in 3176 BCE was followed by Kali Yuga Era calendar starting 3102 BCE? This date occurred in the life-time of Śrī Kr̥ṣṇa who lived through the Kali Yuga and exited in 3031 a year after the Yadava Civil War. See: Krishna avatāra occurs between 3112 and 3031 BCE --ज्योतिष view presented by Prof. Srinivasa Raghavan https://tinyurl.com/yhjdrn88 --I submit that the Kali Yuga Era calendar start year 3102 is related to the manifestation of Śrī Kr̥ṣṇa avatāra, recording the killing of Kamsa by a 11-year young Kr̥ṣṇa evidencing his Kr̥ṣṇa avatāra, divine manifestation. This event occurred to infuse an ethic in sovereigns; this is explained by Śrī Kr̥ṣṇa. -- I submit that the Kali Yuga Era start date 3102 of the Calendar is NOT related to the end of Kr̥ṣṇa avatāra with the ascent of Kr̥ṣṇa to heaven in 3031 BCE. -- The start date of 3102 is chosen by astronomers because of the unique assemblage of planets in that year, a year in which the divine manifestation event occurred -- वसुदेवसुतं देवं कंस चाणूर मर्दनम् । There is another ephocal reason which is related to the restoration of ethical behaviour by sovereign rulers, kings; Kamsa had transgressed the ethical responsibility and became an embodiment of unethical rule. Kamsa dethroned his own father Ugrasena. Kamsa became tyrant ruler of the Vrishni kingdom with its capital at Mathura. Killing of Kamsa occurred in 3102 BCE and is narrated in Udyoga Parva, by daśārha who is Kṛṣṇa https://tinyurl.com/mnf82tbe This episode explains the significance of the killing of Kamsa, an episode recollected when Bhishma expresses his anguish at Duryodhana's irresponsible behaviour.Kr̥ṣṇa responds and comments on the behaviour of Duryodhana and suggests that time has come for Kuru elders to forcibly seize and bind the wicked king Duryodhana:“…this is great transgression, of which all the elders of the Kuru race are becoming guilty, for they do not forcibly seize and bind this wicked king in the enjoyment of sovereignty. Ye chastiser of foes, I think the time hath come for doing this. Then, he goes on to explain the thrilling episode of a 11-year old son of Devaki killing Kamsa. This killing of Kamsa is clearly an epochal event which happened in 3102 BCE when Kr̥ṣṇa was 11 years’ young. This may explain why the Hindu tradition chose the date 17/18 February 3102 BCE as the date of start of Kali Yuga. Source. KD Abhyankar and GB Bhallabh --ṛtv-ij m. (k) a priest (usually four are enumerated, viz. Hotṛ, Adhvaryu, Brahman, and Udgātṛ; each of them has three companions or helpers, so that the total number is sixteen, viz. hotṛ, Maitrāvaruṇa, Acchāvāka, Grāva-stut; adhvaryu, Prati-prasthātṛ, Neṣṭṛ, Un-netṛ; brahman, Brāhmaṇācchaṉsin, Agnīdhra, Potṛ; udgātṛ, Prastotṛ, Pratihartṛ, Subrahmaṇya, ĀśvŚr. iv, 1, 4-6 ), RV. ; AV. ; TS. ; ŚBr. ; KātyŚr. सप्तर्षि पु० ब० व० । सप्त ऋषयः संज्ञात्वात् कर्म० । “मरीचि-रत्रिः पुलहः पुलस्त्यः क्रतुरङ्गिराः । वशिष्ठश्चमहाभाग! सप्तैते ब्रह्मणः सुताः” इत्युक्तेषु सप्तसु ऋषिषु ।मन्वन्तरभेदे तेषा नामभेदा ऋषिशब्दे उक्ता १४५३ पृ०दृश्या । सप्तर्षिमण्डल त्रि० ६ त० । आकाशे नित्यं ध्रुवनक्षत्रपरि-भ्र मके नक्षत्रसप्तकात्मके नक्षत्रमण्डलभेदे “सप्तर्षिमण्डलंतस्माद्दृश्यते सर्वकोपरीति” पुराणम् तच्चारादिऋषिशब्दे १४५२ पृ० दृश्यम् ।--वाचस्पत्यम् सप्तर्षयः, पुं, भूम्नि, (सप्त ऋषयः ।) सप्तसंख्यकर्षयःतेषां नामानि यथा । मरीचिः १ अत्रिः २अङ्गिराः ३ पुलस्त्यः ४ पुलहः ५ क्रतुः ६ वशिष्ठः ७ ।इत्यमरः ॥ अपि च ।“मप्तर्षिमण्डलं तस्माद्दृश्यते सर्व्वतोपरि ।तत्र सप्तर्षयः सन्ति विनियुक्ताः प्रजासृजा ॥मरीचिरत्निः पुलहः पुलस्त्यः क्रतुरङ्गिराः ।वशिष्ठश्च महाभाग ब्रह्मणो मानसाः सुताः ॥सप्तब्राह्मण इत्येते उच्यन्ते ब्रह्मवादिभिः ।संभूतिरनसूया च क्षमा प्रीतिश्च सन्नतिः ॥अरुन्धतिस्तथा लज्जा तत्पत्न्यौ लोकमातरः ।एतासां तपसा चैतद्धार्य्यते भुवनत्रयम् ॥सन्ध्यात्रयमुपासीना गायत्त्रीजपतत्पराः ।तस्मिन्लोके वसन्त्येते ब्राह्मणाः ब्रह्मवादिनः ॥”इति पाद्मे स्वर्गखण्डे ११ अध्यायः ॥(प्रतिमन्वन्तरे सप्तर्षयो भिन्ना एवासन् । तद्-वृत्तान्तस्तु ऋषिशब्दे द्रष्टव्यः ॥)--शब्दकल्पद्रुमः In traditional Hindu astronomy, seven stars of Ursa Major are identified with the names of Saptarṣi. In ancient Indian astronomy, the asterism of the Big Dipper (part of the constellation of Ursa Major) is called saptarishi, with the seven stars representing seven rishis, namely "Vashistha", "Marichi", "Pulastya", "Pulaha", "Atri", "Angiras" and "Kratu". There is another star slightly visible within it, known as "Arundhati". Arundhati and Vashishtha are married, and together form the Mizar double. Saptarishis in each manvantara of the current kalpa (Śveta-Vārāha Kalpa) Manu (manvantara) Saptarishis Svayambhuva Marichi, Atri, Angiras, Pulaha, Kratu, Pulastya, and Vasishtha Svarocisha Urja, Stambha, Prana, Nanda, Rishabha, Nischara and Arvarivat Uttama Kaukundihi, Kurundi, Dalaya, Sankha, Pravahita, Mita and Sammita (Sons of Vasistha) Tapasa/Tamasa Jyotirdhama, Prithu, Kavya, Chaitra, Agni, Vanaka and Pivara Raivata Hirannyaroma, Vedasrí, Urddhabahu, Vedabahu, Sudhaman, Parjanya and Mahamuni Chakshusha Sumedhas, Virajas, Havishmat, Uttama, Madhu, Abhinaman, and Sahishnnu Vaivasvata (current) Jamadagni, Kashyapa, Atri, Vashista, Gautama, Vishvamitra, Bharadvaja Surya-savarni Diptimat, Gslava, Parasurama, Kripa, Drauni or Ashwatthama, Vyasa and Rishyasringa Daksha-savarni Savana, Dyutimat, Bhavya, Vasu, Medhatithi, Jyotishman, and Satya Brahma-savarni Havishman, Sukriti, Satya, Apammurtti, Nabhaga, Apratimaujas and Satyaketu Dharma-savarni Nischara, Agnitejas, Vapushman, Vishnu, Aruni, Havishman and Anagha Rudra-savarni Tapaswi, Sutapas, Tapomurti, Taporati, Tapodhriti, Tapodyuti and Tapodhana Deva-savarni Nirmoha, Tatwadersin, Nishprakampa, Nirutsuka, Dhritimat, Avyaya and Sutapas Indra-savarni Agnibshu, Suchi, Aukra, Magadha, Gridhra, Yukta and Ajita Wilson, Horace Hayman; trans. (1840) "Vishńu Puráńa", Sacred-Texts.com. Contains an account of the several Manus and Manwantaras. https://en.wikipedia.org/wiki/Saptarishi Saptarṣi maṇḍala; Ursa Major Constellation As many of its common names allude, its shape is said to resemble a ladle, an agricultural plough, or wagon. In the context of Ursa Major, they are commonly drawn to represent the hindquarters and tail of the Great Bear. Starting with the "ladle" portion of the dipper and extending clockwise (eastward in the sky) through the handle, these stars are the following: • α Ursae Majoris, known by the Arabic name Dubhe ("the bear"), which at a magnitude of 1.79 is the 35th-brightest star in the sky and the second-brightest of Ursa Major. • β Ursae Majoris, called Merak ("the loins of the bear"), with a magnitude of 2.37. • γ Ursae Majoris, known as Phecda ("thigh"), with a magnitude of 2.44. • δ Ursae Majoris, or Megrez, meaning "root of the tail," referring to its location as the intersection of the body and tail of the bear (or the ladle and handle of the dipper). • ε Ursae Majoris, known as Alioth, a name which refers not to a bear but to a "black horse," the name corrupted from the original and mis-assigned to the similarly named Alcor, the naked-eye binary companion of Mizar.[8] Alioth is the brightest star of Ursa Major and the 33rd-brightest in the sky, with a magnitude of 1.76. It is also the brightest of the chemically peculiar Ap stars, magnetic stars whose chemical elements are either depleted or enhanced, and appear to change as the star rotates.[8] • ζ Ursae Majoris, Mizar, the second star in from the end of the handle of the Big Dipper, and the constellation's fourth-brightest star. Mizar, which means "girdle," forms a famous double star, with its optical companion Alcor (80 Ursae Majoris), the two of which were termed the "horse and rider" by the Arabs. The ability to resolve the two stars with the naked eye is often quoted as a test of eyesight, although even people with quite poor eyesight can see the two stars. • η Ursae Majoris, known as Alkaid, meaning the "end of the tail". With a magnitude of 1.85, Alkaid is the third-brightest star of Ursa Major. https://en.wikipedia.org/wiki/Ursa_Major The earliest list of the Seven Rishis is given by Jaiminiya Brahmana 2.218–221: Agastya, Atri, Bhardwaja, Gautam, Jamadagni, Vashistha and Vishvamitra followed by Brihadaranyaka Upanisad 2.2.6 with a slightly different list: Atri, Bharadvaja, Gautama, Jamadagni, Kashyapa, Vashistha and Vishwamitra. The late Gopatha Brahmana 1.2.8 has Vashistha, Vishvamitra, Jamadagni, Gautama, Bharadvaja, Gungu, Agastya and Kashyapa. Story of Parīkṣit A brilliant King of Candravaṃśa. He was the grandson of Arjuna and son of Abhimanyu. (For genealogy see under Abhimanyu). Birth. Parīkṣit was the son born to Abhimanyu of Uttarā. This was a still-born child and it was Śrī Kṛṣṇa who gave it life. There is a story in Mahābhārata about this: Uttarā, wife of Abhimanyu, was pregnant when the war between the Pāṇḍavas and Kauravas started at Kurukṣetra. Aśvatthāmā, son of Droṇa, entered the camp of the Pāṇḍavas at night and slew Dhṛṣṭadyumna. He then sent the most fierce Brahmaśirāstra (missile of Brahmaśira) to exterminate the Pāṇḍavas. To face it and oppose it Arjuna also sent an equally fierce Brahmaśirāstra. The sight of two such powerful weapons opposing each other made all the sages anxious and they led by Vyāsa entered the field and requested them to withdraw their missiles. It was in vain. The missile of Aśvatthāmā went and struck the womb of Uttarā. Once when the Pāṇḍavas after their exile were staying in the village of Upaplavya a brahmin had predicted to Uttarā that at the fag end of the life of the Pāṇḍavas Uttarā would bear a son who would be tested even while in her womb and that the child should be named Parīkṣit. (Parīkṣā = test).
2023
The antiquity and the chronology of ancient Indian civilization can be presented in Seven distinct stages as follows: 1. Early Vedic Period (14500-11500 BCE) 2. Vedic Period (11500-10500 BCE) 3. Post Vedic Period (10500-6777 BCE) 4. The 28 th Treta Yuga Period (6777-5577 BCE) and the Ramayana Era (5677-5577 BCE) 5. The 28 th Dvapara Yuga Period (5577-3177 BCE) and the Mahabharata Era (3162 BCE) 6. The 28 th Kaliyuga Period (from the 32 nd century BCE onwards) and the Mahabharata Era: From Mahabharata War (3162 BCE) to King Vikramaditya (1 BCE) 7. The Medieval Period (from 1 CE to 1761 CE)
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- A., VII (2001) Cribb for granting access to tbe K~fu.!a coins collection in the British Museum, and for pointing out the latest literature on tbe subject. Notes
- For the original publication see Sims-Willams & Cribb 1995/96; a French version in Sims-Williams 1996; a critical evalutation in Fussman 1998; cf. also Mukherjee 1995 [sic; appeared 1999]; for an encompasing bibliograph¥ of recent research cf. Fussman 1987.
- 's coins (Sims-Williams/Cribb 1995/96:140b,c, 141a), read as takto by Cribb. On some others, unpublished so far, the name ends in takho, aspirated, without the ma. The Ma~ pedestal clearly has [--]ma tak<;1;lma (Fussman 1998:607). It is obvious that takho and tak<;u are adaptations to the same phonetic original; the unaspirated variety, however, seems nearer to the Bactrian form uemo taktu, which Sims-Williams holds ascertained (1995/6:96, n.3; but cf. Fussman 1998:615). There is an unpublished Buddha statue at the Army Museum, Rawalpindi, not on display; its inscription is found as the "Nowshera pedestal inscription" in Konow 1929:134. Konow read dhivhakarasa takhtidre/}-a karide. Some characters are written rather carelessly. Nonetheless, the end of the text can be restored as takhto danamukho. More difficult is the beginning, containing the title. Konow's dhivhakara is impossible, since the second character is not vha, and the third can bqa, or spa or ka. Maybe the title ends in isparasa. At least, in the proper name the ligatur~ khto is absolutely clear. Could the base be something like tak-tsu (plus a nasal) ? In a recent article Mukherjee (1997-98) rejects any form of takto and presents readings of his own which are hard to digest. Finally, he identifies Vima Ta~uma and Vima Kadphises.
- According to Bivar 1963:501, n. 1 this association goes back to A.K. Narain, The Indo-Greeks, Oxford 1957:144 and R.M. Smith, On the ancient chronology ofIndia, JADS 78.1958:178.
- J. van Lohuizen-de-Leeuw 1949:235ff.; suitably summarized in de Lohuizen-de-Leeuw 1986:passim; cf. Sillomon' 1998:183, n.87. The idea of dropped hundreds is as old as 1874, when E. Thomas interpreted the K~~a dates a'sihose of the Seleucidan era of 312 BC or of the Parthian era of 248 BC (Fleet in JRAS 1913:981); cf. Konow in Konow/van Wijk 1924,71 n. 2.
- Notable exceptions are Bivar 1970: 13f. and Mitra 1996: 72f., who expect all Ku~~a kings from Kani~ka !to Kani~ka 11 to have lived in one single century.
- The proceedings are published in the JRAS 1913 as "The date of Kan~ka", with contributions by F.W. Thomas (627-650, 1011-1042), EJ. Rapson (911-913), J.F. Fleet (913-939, 965-1011), V. Smith (939-942), CD. Bamett (942-
- L.A. Waddell (945-952), L. Dames (953-960), W. Hoey (960-965). A systematic analysis of the theories advanced is found in Banerji 1908: 27f. For personal memories cf. R.B. Whitehead 1968: 1-3.
- E.g. Mbh 5. 62, 25 vrddho bhavati vai yuva; for the predicative nominative cf., e.g., Sen 1926-27:348. 11) Salomon 1998: 184.
- It has this meaning in the date yate'fu catur!fukJ:te'fu sate'fu ( .. ,) vatsare'fu in the Gandghar stone inscription, Fleet 1888:75. 13) Last in Gob11999: 162 "third century A.D.", earlier he spoke of 225 A.D. (1999: 164).
- An odd ending and a deliberate new era with Kani~ka 11 is expected by Bivar (1963:498, n. 4). 15) For the source text see Ziircher 1968: 371.
- Fussman 1998: 640, while defending Kani~ka as the originator of an era starting in AD 78, maintains that "cette date seule, a laquelle rien ne s'oppose, permet de resoudre l'enigme de l'ere saka".
- Sachau 1914, II: 6; these astronomers start the saka year with caitra, Sachau 1914, II: 8.
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Harry Falk

