Sydney:12/24 22:26:56

Tokyo:12/24 22:26:56

Hong Kong:12/24 22:26:56

Singapore:12/24 22:26:56

Dubai:12/24 22:26:56

London:12/24 22:26:56

New York:12/24 22:26:56

2026-02-19 Thursday

2026-02-22

11:03:15

The average operating rate of PAJ refineries in Japan for the week ending February 14

Previous : 89.20% Forecast : -

Published Value 89%

Previous

11:03:13

Japan's PAJ kerosene inventory changes for the week ending February 14 -KER

Previous : -17.06 Forecast : -

Published Value -17.76

Previous

11:03:12

Changes in Japan's PAJ commercial crude oil inventories for the week ending February 14

Previous : 16.78 Forecast : -

Published Value -36.46

Previous

11:03:12

Changes in PAJ gasoline inventories in Japan for the week ending February 14 -GAS

Previous : -7.15 Forecast : -

Published Value 8.23

Previous

09:56:23

[Chinese Researchers Propose New Explanation for the Cause of an Ultra-Long Gamma-Ray Burst] Gamma-ray bursts are among the most violent explosive phenomena in the universe, typically lasting from milliseconds to several minutes. Recently, a new study has provided a fresh perspective on this event. A team from the National Key Laboratory of Particle Astrophysics at the Institute of High Energy Physics, Chinese Academy of Sciences, used a newly developed analytical tool to comprehensively search observational data from satellites such as HXMT and JX3 for 30 days before and after this gamma-ray burst. They discovered that it lasted for 29 hours in the gamma-ray band, breaking the record for the longest gamma-ray burst. Furthermore, the team also found that the accompanying X-ray radiation exhibited unique time-varying characteristics. Based on these findings, the research team proposed a novel "supergiant self-regulating collapse star model." This model suggests that the progenitor of this gamma-ray burst was a supergiant star with a mass far exceeding that of the Sun. Unlike the progenitors of ordinary gamma-ray bursts, the collapse of a supergiant can last for tens of days. When the supergiant exhausts its fuel, its core first collapses to form a black hole. The black hole rapidly accretes matter from the supergiant's inner layers, generating jets at near-light speed—the source of the gamma-ray burst. During the subsequent accretion process, a slightly slower jet was generated, emitting X-ray radiation. (Xinhua)

09:01:04

The proportion of Swift RMB in global payments in China in January

Previous : 2.73% Forecast : -

Published Value 3.13%

Previous

Real-Time Popular Commodities

Instrument Current Price Change

XAU

5098.85

103.02

(2.06%)

XAG

84.227

5.873

(7.50%)

CONC

66.31

-0.09

(-0.14%)

OILC

71.58

-0.31

(-0.44%)

USD

97.807

-0.045

(-0.05%)

EURUSD

1.1785

0.0012

(0.10%)

GBPUSD

1.3484

0.0021

(0.16%)

USDCNH

6.8955

-0.0024

(-0.04%)