Sounding the Stars - Asteroseismology of Stars with Sun-like Oscillations
Sounding the Stars - Asteroseismology of Stars with Sun-like Oscillations
批准号:
ST/F002041/1
负责人:
William Chaplin
金额:
$42.75万
依托单位:
依托单位国家:
英国
项目类别:
Research Grant
财政年份:
2009
资助国家:
英国
项目状态:
已结题
起止时间:
2009 至 --
中文摘要
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英文摘要
Stars are building blocks of the universe, and are crucial sources of energy for giving conditions which can support life. Knowledge on how stars are born, live, evolve, and then die, underpins much of our understanding of the universe. Our research will 'peer' deep inside stars to understand how they work, and to add previously unknown knowledge on the life-cycles of the stars. Our research will also provide important information for 'planet hunters', who are searching for potentially habitable planets like Earth orbiting other stars. We are interested in stars that vibrate gently like our own star, the Sun. Although you cannot see it without special equipment, the Sun is shaking. Bubbling motion just under the visible surface of the Sun is constantly feeding in energy, and the Sun responds by vibrating just like a (very) large musical instrument. The 'notes' of the Sun's music are very interesting to astronomers. They are made by sound waves, some of which have travelled deep inside the Sun, and their frequencies (the pitch of the notes) depend on conditions they meet on the way. For example, the frequencies depend on the density and temperature of the material inside the Sun, and studying them allows astronomers to essentially get an ultrasound scan of our nearest star by 'sounding' its interior. Because the Sun is a ball of largely ionized gas, when it shakes it gently oscillates. The oscillations make the surface move to and fro at a couple of metres per second (a slow walking pace!), and it takes about 5 minutes to go through a complete cycle. Just detecting this small movement is very hard, and takes specially designed instruments. But doing so for other stars is much, much harder again, because they are many orders of magnitude fainter than the Sun. The solar oscillations were discovered in the 1960s, and it took until the mid to late 1990s for ingenious astronomers to discover oscillations like them on another star. There are now more than a dozen stars that have been observed to oscillate like the Sun. They range from stars that both look like, and are at the same points in their life cycles, as the Sun; through to much more mature stars that have expanded in their old ages to become 'red giants'. We now stand on the threshold of an exciting expansion in observations of the oscillations on other stars, with the launch of new space missions, and continuation of observations from telescopes around the world. These observations will allow astronomers to test their theories of how all stars live and evolve, by peering into their interiors, like we can for the Sun. That is what we propose to do. We will use the exciting new data from telescopes and space missions to 'sound the stars'. Our work will also go hand-in-hand with searches for Earth-like planets around other stars. That is because we will use data from NASA's Kepler space mission, which will look for oscillations and hunt for planets, at the same time. Our work will help to reveal the nature of stars around which planets are found, and will also give us more information on the planets themselves.
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DOI:
10.1007/s10509-009-0164-x
发表时间:
2010-07
期刊:
Astrophysics and Space Science
影响因子:
1.9
作者:
[S. Basu;W. Chaplin;Y. Elsworth]
通讯作者:
S. Basu;W. Chaplin;Y. Elsworth
Solar-like oscillations in HD 181420: data analysis of 156 days of CoRoT data
HD 181420中的类太阳振荡:156天CoRoT数据的数据分析
DOI:
10.1051/0004-6361/200911937
发表时间:
2009
期刊:
Astronomy & Astrophysics
影响因子:
6.5
作者:
[Barban C]
通讯作者:
Barban C
SOLAR-LIKE OSCILLATIONS IN LOW-LUMINOSITY RED GIANTS: FIRST RESULTS FROM KEPLER
低光度红巨星中的类太阳振荡:开普勒的第一个结果
DOI:
10.1088/2041-8205/713/2/l176
发表时间:
2010
期刊:
The Astrophysical Journal
影响因子:
--
作者:
[Bedding T]
通讯作者:
Bedding T
DOI:
10.1088/0004-637x/710/2/1596
发表时间:
2009-09
期刊:
The Astrophysical Journal
影响因子:
--
作者:
[S. Basu;W. Chaplin;Y. Elsworth]
通讯作者:
S. Basu;W. Chaplin;Y. Elsworth
A MULTI-SITE CAMPAIGN TO MEASURE SOLAR-LIKE OSCILLATIONS IN PROCYON. II. MODE FREQUENCIES
测量南河三星中类太阳振荡的多站点活动。
DOI:
10.1088/0004-637x/713/2/935
发表时间:
2010
期刊:
The Astrophysical Journal
影响因子:
--
作者:
[Bedding T]
通讯作者:
Bedding T
共 8 条
Refresh, Continuation, and Science Exploitation of the Birmingham Solar-Oscillations Network (BiSON)
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批准号:ST/Z000025/1
-
项目类别:Research Grant
-
资助金额:$94.54万
-
财政年份:2024
-
负责人:William Chaplin
-
依托单位:
Helioseismology at Birmingham and Queen Mary
-
批准号:ST/V000500/1
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项目类别:Research Grant
-
资助金额:$74.02万
-
财政年份:2021
-
负责人:William Chaplin
-
依托单位:
Asteroseismology and Exoplanets at Birmingham and Queen Mary
-
批准号:ST/V000519/1
-
项目类别:Research Grant
-
资助金额:$59.81万
-
财政年份:2021
-
负责人:William Chaplin
-
依托单位:
Helioseismology at Birmingham and Queen Mary
-
批准号:ST/R000417/1
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项目类别:Research Grant
-
资助金额:$47.76万
-
财政年份:2018
-
负责人:William Chaplin
-
依托单位:
Asteroseismology and Helioseismology at Birmingham and Queen Mary
-
批准号:ST/M00077X/1
-
项目类别:Research Grant
-
资助金额:$128.19万
-
财政年份:2015
-
负责人:William Chaplin
-
依托单位:
国内基金
海外基金
基于STARS分析的渤海营养状态转换及其生态效应研究
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批准号:41906044
-
项目类别:青年科学基金项目
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资助金额:25.0万元
-
批准年份:2019
-
负责人:辛明
-
依托单位:
STARS-SRF信号通路在脂代谢中的分子调节机制
-
批准号:31171131
-
项目类别:面上项目
-
资助金额:60.0万元
-
批准年份:2011
-
负责人:金万洙
-
依托单位: