Mashable 01月04日
Scientists predicted this star would explode. Its bucked expectations.
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耀星T Coronae Borealis (T CrB) 是一颗每80年左右爆发一次的重复新星系统,由一颗白矮星和一颗红超巨星组成。白矮星不断吸积红超巨星的气体,当积累到足够量时,会在其表面引发剧烈的热核反应,形成新星爆发。尽管科学家预测它可能在2024年爆发,但目前仍未出现。其爆发时间难以精确预测,因为气体积累的速度未知。尽管如此,天文学家已确定其在夜空中的位置,位于北冕座,可在晴朗的夜晚通过寻找大角星和织女星来定位。爆发时,它将肉眼可见,但仅持续不到一周。

🌟T CrB是一颗罕见的重复新星,大约每80年爆发一次,其爆发源于白矮星吸积红超巨星的气体,引发热核反应。

🌌尽管科学家预测2024年可能爆发,但其具体时间难以预测,因为气体积累速度未知,这使得T CrB的行为难以捉摸。

🔭观测者可以在夜空中寻找北冕座,它位于武仙座的西部,呈马蹄形曲线,可以通过大角星和织女星定位,在爆发时可肉眼观测到。

⏱️T CrB爆发后,肉眼可见的时间很短,只有不到一周,这与中世纪甚至更早的观测情况类似,需要快速行动才能捕捉到这一天文奇观。

For centuries, stargazers have watched a new star light up in the sky. Just days later, it vanishes.

Today we call the star system responsible T Coronae Borealis, "T CrB" for short, or the "Blaze Star." It fires up around every 80 years, and NASA noted that astronomers expected to see the star appear around the summer of 2024. It's now 2025. What gives?

This repeating event — occurring 3,000 light-years from Earth — is triggered by two interacting, orbiting stars. An Earth-sized star called a white dwarf (the dense remnants of an exploded sun-like star) is ripping gas away from a nearby red supergiant star. Years pass, and prodigious amounts of gas amass on the white dwarf's surface. Under such extreme heat and pressure, the surface blows in a violent thermonuclear reaction, called a nova.

But a precise deep space prediction is difficult.

"We’re waiting for a 'new' star to briefly make an appearance, but we don’t know exactly when it will occur. The star is pulling material from a companion star, and over decades it collects enough to trigger an eruption," NASA recently explained in a post. "But we don’t know how fast the material is piling up!"

The space agency added that "we have clues that it may erupt soon, but 'soon' could mean today or next year!" (That's "next year" as in 2026.)

Although scientists had high hopes for a 2024 spectacle, the star's elusive behavior isn't too surprising. We're still learning about these cosmic explosions.

"Recurrent novae are unpredictable and contrarian," Dr. Koji Mukai, a NASA astrophysicist, said in a 2024 statement. "When you think there can’t possibly be a reason they follow a certain set pattern, they do — and as soon as you start to rely on them repeating the same pattern, they deviate from it completely. We’ll see how T CrB behaves."

How to see T Coronae Borealis when it explodes

Although T Coronae Borealis' timing isn't certain, astronomers know for certain where it'll appear in the night sky. NASA explains:

What should stargazers look for? The Northern Crown is a horseshoe-shaped curve of stars west of the Hercules constellation, ideally spotted on clear nights. It can be identified by locating the two brightest stars in the Northern Hemisphere — Arcturus and Vega — and tracking a straight line from one to the other, which will lead skywatchers to Hercules and the Corona Borealis.

(In the summer months, the Northern Crown appears in the sky after sunset, which makes ideal viewing.)

But you'll have to act fast. After erupting and appearing, it'll only be visible with the naked eye for less than a week, similar to how watchers viewed it long ago, during the Middle Ages, if not much earlier.

The location of T Coronae Borealis in the night sky. Credit: NASA

If it behaves as (generally) expected, the exploded star will reappear in another 80 or so years, after prodigious amounts of stellar gas settle onto its surface.

Then, boom.

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耀星 T CrB 新星爆发 天文学 北冕座
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