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Scientists studying the Tarantula Nebula1 say they have gained a greater understanding of how stars form.
The researchers also got a beautiful image of a large cloud of gas and dust that neighbors the Milky2 Way galaxy3.
Researchers recently said their observations offered information about the connection between two competing processes – gravity and feedback. Gravity is the force that drives star formation, while the competing process, known as feedback, refers to the huge amounts of energy that large young stars introduce into their nearby environments to limit star growth.
The Tarantula Nebula is an area of stars, gas and dust 600 light-years across. A light year is the distance light travels in a year - about 9.5 trillion kilometers.
The Tarantula Nebula's official name is 30 Doradus. It is about 170,000 light years from Earth.
It is called the Tarantula Nebula because its paths of gas, dust and stars look like spider legs. The nebula's gas mixture is much like that of the early universe: mostly hydrogen and helium.
The European Southern Observatory4 released a Tarantula Nebula image showing thin gas clouds that may be the remains5 of larger ones. Scientists think great bursts of energy from large young stars may have torn apart the gas clouds.
Guido De Marchi was a co-writer of the research published in The Astrophysical Journal and presented the work at a meeting of the American Astronomical6 Society.
"We see stars forming where there is a lot of gas and dust available, and there is definitely a lot of it in the Tarantula Nebula," De Marchi said.
Researchers were helped by observations from the Chile-based ALMA telescope.
De Marchi explained that "Stars form when gas clouds collapse7 under their own gravity and the gas gets denser9 and denser."
He added that these gas clouds "contract and warm up until the core is hot enough to start the stellar engine, an immense nuclear reactor10."
Immense means extremely large.
De Marchi said that scientists used to believe that when very large stars – those 100 times bigger than the sun – begin to form they release so much energy that they shut off the fuel for more stars to form.
De Marchi added, "The beautiful observations of the Tarantula Nebula obtained with ALMA now show that where the gas is dense8 enough it continues to fall ... and new stars can keep forming. This is interesting and new."
The process De Marchi talked about is called feedback, in which large young stars release large amounts of energy in the form of photons and high-speed particles. The nebula's composition has led to the creation of particularly large stars, some 200 times as massive as our sun.
Tony Wong, the lead writer of the report, said Tarantula Nebula is the most extreme feedback environment scientists can observe.
"One of the big mysteries in astronomy is why we are still able to witness stars forming today," Wong said.
He continued, "Observations with ALMA can shine a light on what is happening deep within clouds and help us understand how gravity and feedback compete for influence to keep the rate of star formation under control."
Words in This Story
formation — n. something that is formed or created; the act of forming or creating something
composition — n. the way in which something is put together or arranged
contract — v. to become smaller
stellar — adj. of or relating to the stars
photon — n. a tiny particle of light or electromagnetic radiation
1 nebula | |
n.星云,喷雾剂 | |
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2 milky | |
adj.牛奶的,多奶的;乳白色的 | |
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3 galaxy | |
n.星系;银河系;一群(杰出或著名的人物) | |
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4 observatory | |
n.天文台,气象台,瞭望台,观测台 | |
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5 remains | |
n.剩余物,残留物;遗体,遗迹 | |
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6 astronomical | |
adj.天文学的,(数字)极大的 | |
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7 collapse | |
vi.累倒;昏倒;倒塌;塌陷 | |
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8 dense | |
a.密集的,稠密的,浓密的;密度大的 | |
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9 denser | |
adj. 不易看透的, 密集的, 浓厚的, 愚钝的 | |
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10 reactor | |
n.反应器;反应堆 | |
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