Event research Shadow of Intent - Imperium Delirium North American Tour 2026
Shadow of Intent - Imperium Delirium North American Tour 2026 tickets are on sale right now.
Are Shadow of Intent - Imperium Delirium North American Tour 2026 tickets likely to be profitable in Cincinnati, OH?
There are 5 presales for this event - we have 4 unique passwords for these presales.
Shadow of Intent - Imperium Delirium North American Tour 2026
Bogart's
Cincinnati, OH
May 12 Tue • 2026 • 6:00pm
Alternative Rock | Metal | Hard Rock/Metal | Event
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1,500
Capacity
Shadow of Intent - Imperium Delirium North American Tour 2026 at the Bogart's, Cincinnati, OH
Presale Passwords & On Sale Times
Shadow of Intent - Imperium Delirium North American Tour 2026
| Public Onsale | Dec 5 Fri 2025 | 10:00am | to | May 12 Tue 2026 | 8:00pm | |||
 Citi® Cardmember Presale |
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Dec 4 Thu 2025 | 10:00am | to | Dec 4 Thu 2025 | 10:00pm | ||
 Live Nation Presale |
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Dec 4 Thu 2025 | 10:00am | to | Dec 4 Thu 2025 | 10:00pm | ||
 Ticketmaster Presale |
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Dec 4 Thu 2025 | 10:00am | to | Dec 4 Thu 2025 | 10:00pm | ||
| Citi® Cardmember Preferred Tickets |
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Dec 5 Fri 2025 | 10:00am | to | May 5 Tue 2026 | 10:00pm | ||
 T-Mobile® Concert Perks + Fast Lane |
Dec 5 Fri 2025 | 10:00am | to | May 9 Sat 2026 | 6:00pm | |||
Tour Schedule
Shadow of Intent - Imperium Delirium North American Tour 2026
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Wikipedia Bio
A synestia is a hypothesized structure for the debris field generated by the collision of planets: a rapidly spinning doughnut-shaped mass of vaporized rock. The term was coined in 2017 by Sarah T. Stewart-Mukhopadhyay, taken from Hestia, goddess of the hearth, combined with syn- meaning together.[1] In computer simulations of giant impacts of rotating objects, a synestia can form if the total angular momentum is greater than the co-rotational limit.[2] Beyond the co-rotational limit, the velocity at the equator of a body would exceed the orbital velocity.[3]
In the case of a synestia, the result is an inner region rotating at a single rate with a loosely connected torus orbiting beyond it.[4] Synestias also have differences in the mantles, both thermally and in their composition, from previous terrestrial evolution models due partially to a lower interior pressure.[5]
- ^ "Where did the Moon come from? A new theory | Sarah T. Stewart". YouTube.
- ^ Boyle, Rebecca (23 June 2017) [25 May 2017]. "Huge impact could have smashed early Earth into a doughnut shape". New Scientist. Retrieved 7 June 2017.
- ^ Gough, Evan (24 May 2017). "Scientists propose a new kind of planet: A smashed-up torus of hot, vaporized rock". Universe Today. Retrieved 7 June 2017.
- ^ Lock, Simon J.; Stewart, Sarah T. (2017). "The structure of terrestrial bodies: Impact heating, corotation limits and synestias". Journal of Geophysical Research: Planets. 122 (5): 950–982. arXiv:1705.07858. Bibcode:2017JGRE..122..950L. doi:10.1002/2016JE005239. S2CID 118959814.
- ^ Lock, Simon J. (2018). The Formation, Structure and Evolution of Terrestrial Planets. Graduate School of Arts & Sciences (Ph.D. thesis). Harvard University.
Source: Wikipedia