Signum Explorer - Transaction #5489816904304865031

Transaction ID
5489816904304865031

Height	406626 356628 Block Confirmations
Type	Ordinary Payment
Timestamp	2 years, 9 months ago (2022-03-22 19:53:24 UTC)
From	TS-K37B-9V85-FB95-793HN OHAGER-K3
To	TS-QAJA-QW5Y-SWVP-4RVP4 ohager
Value	1.0 TSIGNA ($0.123)
Fee	0.12 TSIGNA ($0.0148)
Version	2
Deadline	1440
Block Timestamp	2 years, 9 months ago (2022-03-22 19:53:28 UTC)
EC Block ID	5214348882899120974
EC Block Height	406616
Has message	yes
Has encrypted message	no
Has Public Key Announcement	yes
Has Encrypttoself Message	no
Sender Public Key	7210B8941929030324540238450E985899989A7AD0267E0C76F668FDE3B1016B
Signature	FB5D9DB1BC45E29D7AA0ADED476492D4F7B7A4CB6D88BBEAE7D33999E703CA03D05BA8B4A75B630701BD660F50AFE55E450B9235C1A3B47C12CDA3944CA6AF9A
Full Hash	07AF065F63BF2F4CF14FE92490919F309AEA7A81D267E2C8F7B1682FD814A192
Message	A black hole is a region of spacetime where gravity is so strong that nothing — no particles or even electromagnetic radiation such as light — can escape from it.[2] The theory of general relativity predicts that a sufficiently compact mass can deform spacetime to form a black hole.[3][4] The boundary of no escape is called the event horizon. Although it has an enormous effect on the fate and circumstances of an object crossing it, it has no locally detectable features according to general relativity.[5] In many ways, a black hole acts like an ideal black body, as it reflects no light.[6][7] Moreover, quantum field theory in curved spacetime predicts that event horizons emit Hawking radiation, with the same spectrum as a black body of a temperature inversely proportional to its mass. This temperature is of the order of billionths of a kelvin for stellar black holes, making it essentially impossible to observe directly.
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Transaction ID 5489816904304865031

Transaction ID
5489816904304865031