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Space Station Experiment To Probe Origins of Elements

Astronomer Carl Sagan put it best: “We’re made of star stuff.” The atoms that make up the chemicals of our bodies didn’t originate on Earth; they came from deep space. The big bang created hydrogen, helium, and a little bit of lithium, but heavier atoms – the ones essential for life – came from processes related to stars.


Scientists can now probe deeper. Which kinds of stellar processes produce which elements? And which kinds of stars are involved?


A new experiment called TIGERISS, envisioned for the International Space Station, aims to find out. TIGERISS has been chosen as the latest NASA Astrophysics Pioneers mission.


Pioneers are small-scale astrophysics missions that enable innovative investigations into cosmic phenomena. They may include experiments designed to fly on small satellites, scientific balloons, the space station, and payloads that could orbit or land on the Moon.


Earlier this year, the four previous Pioneers mission concepts, chosen in January 2021, were given the green light to move forward with construction and have been approved to fly later this decade.


“The Pioneer missions are an invaluable opportunity for early to mid-career scientists to conduct compelling astrophysics investigations, while gaining real experience in building space-based instrumentation,” said Mark Clampin, director of the astrophysics division at NASA Headquarters in Washington. “With TIGERISS, the Pioneers expand their reach to the space station, which offers a unique platform for exploring the universe.”

美国国家航空航天局华盛顿总部天体物理部门主任Mark Clampin说:“对于职业生涯早期到中期的科学家来说,‘先锋号’任务是一个非常宝贵的机会,可以进行引人注目的天体物理学研究,同时获得建造天基仪器的真正经验。”“通过TIGERISS,先驱者将触角延伸到了空间站,这为探索宇宙提供了一个独特的平台。”

TIGERISS Principal Investigator Brian Rauch, research associate professor of physics at Washington University in St. Louis, has been working on questions of elemental origins and high-energy particles since he was an undergraduate there. For nearly three years in college, Rauch worked on a particle detector called Trans-Iron Galactic Element Recorder, or TIGER. The experiment had its first flight on a balloon in 1995; long-duration balloon flights also launched a version of TIGER from Antarctica in 2001 to 2002 and 2003 to 2004.

TIGERISS的首席研究员Brian Rauch是圣路易斯华盛顿大学的物理学研究副教授,他从本科起就一直在研究元素起源和高能粒子的问题。大学期间,劳赫花了近三年的时间研究一种名为“跨铁银河元素记录器”(Trans-Iron Galactic Element Recorder,简称TIGER)的粒子探测器。1995年,该实验在气球上进行了首次飞行;在2001年到2002年以及2003年到2004年,长时间的气球飞行也曾在南极洲发射过一个TIGER版本。

As Rauch progressed in his research career, he helped TIGER evolve into the more sophisticated SuperTIGER. On Dec. 8, 2012, SuperTIGER launched from Antarctica on its first flight, cruising at an average altitude of 125,000 feet and setting a new record for longest scientific balloon flight — 55 days. SuperTIGER also flew for 32 days from December 2019 to January 2020. The experiment measured the abundance of elements on the periodic table up to barium, atomic number 56.


On the International Space Station, the TIGER instrument family will soar to new heights. Without the interference from Earth’s atmosphere, the TIGERISS experiment will make higher-resolution measurements and pick up heavy particles that wouldn’t be possible from a scientific balloon. A perch on the space station will also allow for a larger physical experiment – 3.2 feet (1 meter) on a side – than could fit on a small satellite, increasing the potential size of the detector. And the experiment could last more than a year, compared to less than two months on a balloon flight. Researchers plan to be able to measure individual elements as heavy as lead, atomic number 82.


Star Stuff


All stars exist in a delicate balance – they need to put out enough energy to counteract their own gravity. That energy comes from fusing elements together to make heavier ones, including carbon, nitrogen, and oxygen, which are important for life as we know it. But once a giant star tries to fuse iron atoms, the reaction doesn’t generate enough power to fight gravity, and the star’s core collapses.


This triggers an explosion known as a supernova, in which shock waves cast out all of those heavy elements that had been made in the star’s core. The explosion itself also creates heavy elements and accelerates them to nearly the speed of light – particles that scientists dub “cosmic rays.”


But that’s not the only way heavy atoms can form. When a superdense remnant of a supernova called a neutron star collides with another neutron star, their cataclysmic merger also creates heavy elements.