2024/07/06

The Stars are Comforting

The Stars are Comforting

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Beatrice Hill Tinsley (1941-1981) was a world leader in modern cosmology especially noted for her study of Evolution of Galaxies. Her research on how galaxies evolve over time changed the standard method for determining distances to far galaxies, which, in turn, is significant in determining the size of the universe and its rate of expansion.

Beatrice was also an accomplished violinist who was a foundation member of the NZ National Youth Orchestra. Throughout her busy life she always made time to practice and play chamber music with her friends and attend concerts, and to write home to her family. Music was an important counterbalance to her extraordinary passion and achievements in cosmology.






Nursery of New Stars: A vast nebula called NGC 604, which lies in the neighboring spiral galaxy M33, located 2.7 million light-years away in the constellation Triangulum. This is a site where new stars are being born in a spiral arm of the galaxy. www.nasaimages.org



Beatrice at her debutant ball in 1959.



Approximately 100 million years ago, a smaller galaxy plunged through the heart of Cartwheel galaxy, creating ripples of brief star formation. www.nasaimages.org



The National Youth Orchestra 1959. Beatrice is in the second row from the front wearing a black high-necked top.



Our great galactic neighbour Andromeda brims with young and old stars. www.nasaimages.org



Extract from a letter, 1962.



Gas has been heated to millions of degrees by the violent outflow of matter blasting out of this galaxy. The eruption can be traced back to the central regions of the galaxy where stars are forming at a furious rate, some 10 times faster than in the Milky Way Galaxy. Many of these newly formed stars are very massive and race through their evolution to explode as supernovas. Vigorous mass loss from these stars before they explode, and the heat generated by the supernovas drive the gas out of the galaxy at millions of miles per hour. It is thought that the expulsion of matter from a galaxy during bursts of star formation is one of the main ways of spreading elements like carbon and oxygen throughout the universe. www.nasaimages.org



Extract from a letter, 1962.



Galaxy NGC 2976, located approximately 10 million light-years away in the constellation Ursa Major near the Big Dipper. Unlike other spiral galaxies where the star-forming and dusty regions highlight spiral arms, this galaxy has a rather chaotic appearance. As the "glowing" red emission maps out, Spitzer is able to pierce through dense clouds of gas and dust that comprise the spiral disk, revealing new star formation that is driving the evolution of the galaxy. www.nasaimages.org



Extract from a letter, 1962.



The galaxy cluster Abell 2125. Several massive multimillion degree Celsius gas clouds appear to be in the process of merging. Ten of the point-like sources are associated with galaxies in the cluster and the rest are probably distant background galaxies. The bright gas cloud on the upper left is the core of the cluster and envelopes hundreds of galaxies. www.nasaimages.org



Beatrice with her children, Alan and Terry, 1970.



Located 10 million light-years away in the southern constellation Sculptor, the Silver Dollar galaxy, or NGC 253, is one of the brightest spiral galaxies in the night sky. www.nasaimages.org



String trio, 1970



Bode's Galaxy M81: This galaxy is tilted at an oblique angle on to our line of sight, giving a birds-eye view of the spiral structure. The galaxy is similar to our Milky Way, but our favourable view provides a better picture of the typical architecture of spiral galaxies. M81 may be undergoing a surge of star formation along the spiral arms due to a close encounter it may have had with its nearby spiral galaxy NGC 3077 and a nearby starburst galaxy (M82) about 300 million years ago. M81 is one of the brightest galaxies that can be seen from the Earth. It is high in the northern sky in the circumpolar constellation Ursa Major, the Great Bear. www.nasaimages.org



Beatrice at Yale.



While perhaps not quite as well known as its star-formation cousin Orion, the Corona Australis region (containing, at its heart, the Coronet cluster) is one of the nearest and most active regions of ongoing star formation. At only about 420 light-years away, the Coronet is over three times closer than the Orion nebula is to Earth. The Coronet contains a loose cluster of a few dozen young stars with a wide range of masses and at various stages of evolution, giving astronomers an opportunity to observe embryonic stars simultaneously in several wavelengths. www.nasaimages.org



















The letters of Beatrice Hill Tinsley (1941-1981)

A 20-part series based on the internationally-recognised New Zealand scientist’s letters to her family.

Read by Tina Regtien.

Produced by Adrienne Baron with engineering by Phil Brownlee.

New Zealand's Unknown Genius Beatrice Hill Tinsley


New Zealand's Unknown Genius

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The book Bright Star by Cristine Cole Catley was instrumental in the research for this video.  

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Editing by Noor Hanania
Transcript
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Transcript


0:00
Today I'm walking the trail from Lake Tekapo up to  Ōtehīwai, Mount John. It's a few hours inland from  
0:06
Christchurch, New Zealand, and a place I used to  come a lot as an undergrad studying astronomy at  
0:10
the University of Canterbury. At the top of this  hill are some of New Zealand's biggest telescopes,  
0:15
and so I wanted to take this chance to talk  about one of New Zealand's greatest astronomers.
0:21
She changed the study of galaxies forever, and  she was the first to grasp that galaxies, just  
0:27
like the stars within them, evolve with time. We  are lucky to be able to look at pictures of space,  
0:33
like recent ones from the JWST, and know a  little bit about what we're looking at. Each  
0:39
dot is a galaxy. That's an unfathomable  truth, given how large our own galaxy is.
0:46
And much of the science that goes on today, trying  to understand these dots, was spearheaded by an  
0:52
astronomer from a small New Zealand town.  Her name was Beatrice Hill Tinsley. She  
0:57
was a trailblazer. And as I walk up this hill  today, I'm going to share with you her story.
1:10
Much of what I know about Beatrice I've  learned in this book, Bright Star by  
1:14
Christine Cole Catley. It was a hard book  to find. I got this copy from an old and  
1:18
rare bookstore in Otago and it happens to  be an old library copy. And it's a shame  
1:23
this book isn't more popular because I think  that more people should know about Beatrice.
1:29
She was born Beatrice Hill in England in  1941, but came to New Zealand as a baby  
1:34
and grew up in New Plymouth. As a young girl,  there were a few books about astronomy that  
1:39
really fascinated Beatrice. One in particular  was Fred Hoyle's The Nature of the Universe,  
1:45
which asked questions such as,  how was the universe created?
1:51
At age 14, Beatrice was hungry to know more  and asked to borrow some physics textbooks  
1:56
from her school teacher's bookshelf. She worked  through them by herself. A couple of years later,  
2:02
that same teacher was injured in a  car accident just weeks before the  
2:06
school's final exams. Beatrice led her  class to study without their teacher,  
2:11
and in the final exam, the  students got excellent marks.
2:15
This teacher later said that very occasionally,  you realize you're dealing with a mind that is  
2:20
infinitely superior to your own. Beatrice  came into that category. I would call her a  
2:26
genius. Beatrice graduated at just age 16 from New  Plymouth Girls High School with top marks in her  
2:33
year, and she went on to study at the University  of Canterbury, the same university I went to.
2:39
She didn't like rote learning and preferred to  teach herself interesting ideas. In a letter  
2:44
home from university, she wrote  that she was sick of working for  
2:48
exams and decided to sit in the back of  lectures and work on learning new maths  
2:53
rather than listening to the lecturer mumble  through calculus she had learned at school.
3:02
During her time at Canterbury, Beatrice  decided that she wanted to be a cosmologist,  
3:06
but that wasn't really a topic offered  at the university at that time. This  
3:10
observatory that I'm walking to now  wasn't built when Beatrice was a student,  
3:14
so she had to do a different research  topic for her master's thesis.
3:18
Its title was Theory of the Crystal  Field in Neodymium Magnesium Nitrate.  
3:23
Even though it wasn't the topic that she was  passionate about it gave the added benefit  
3:28
of giving her skills using a computer,  and she was one of the only people in  
3:31
the country who got those kind of skills,  and that helped her later in her career.
3:36
She got all A's at university and was the  only woman in physics at master's level.  
3:41
She also won every academic prize available to  her, including the Haydon Prize for Physics,  
3:47
which I also won 55 years after her. I do  feel connected to Beatrice in lots of little  
3:52
ways. And she also won a postgraduate  scholarship to continue her studies.
3:58
However, her path after university wasn't so  streamlined, and she faced many difficulties  
4:03
in continuing her studies. She got married at  age 20 to fellow physics student Brian Tinsley.  
4:09
They moved together to Dallas, Texas.  At the time, there were anti nepotism  
4:14
laws that prevented both a husband and wife  from being employed at the same institution.
4:19
And Beatrice hadn't known this when she got  married and felt betrayed. It prevented her  
4:24
from continuing her research because Brian  was already employed in Dallas. Feeling  
4:29
like her potential was languishing, Beatrice  took matters into her own hands and decided  
4:34
to find somewhere that would let her do  a PhD, even if it meant a long commute.
4:39
At the University of Austin, a five hour bus ride  away, she managed to convince a professor to give  
4:45
her a chance. They told her that most students  struggled to complete the program in six years,  
4:50
working full time, but she needed  to do it part time, splitting her  
4:55
time between Dallas and Austin. There is a  comment in Catley's book about this time,  
4:59
saying that Beatrice used her scholarship to  pay for all the travel plus Brian having to  
5:04
eat out half the week. This comment disturbed  me a little, I guess it's evident that Brian  
5:09
wouldn't be expected to cook for himself,  and it doesn't sound like Beatrice also  
5:14
got the luxury of eating out. It's only a  small comment, but it does start to speak  
5:18
to the realities of her married life, which she  later described as being like a prison for her.
5:24
Regardless, she did very well at her PhD, and she  astounded the professors and fellow students by  
5:30
scoring the first ever 100 on an exam there.  In a letter home to her New Zealand family,  
5:36
she described the topic of her thesis  by saying, I will be studying a whole  
5:41
lot of different theories of cosmology  to see which is best able to explain  
5:45
the observations made with optical and  radio telescopes on different galaxies.
5:50
The theories are based on Einstein's General  Relativity. Around the time of starting to write  
5:56
up her thesis, Beatrice was thrown a curveball.  An unmarried member of her husband's family  
6:01
became pregnant and at that time, the baby  would need to be adopted out. Beatrice was  
6:07
unexpectedly thrust into motherhood, feeling  compelled to adopt the baby boy, named Allen.
6:13
She wrote up her thesis while taking care of the  baby, and remember how I said most students take  
6:18
six years to finish? Well, Beatrice made such  impressive progress that she was able to finish  
6:23
it in under three years. An examiner at her  oral presentation said it was such powerful  
6:29
work that they should simply award her the PhD  then and there, without asking any questions.
6:35
Although they did continue to ask some, just  to meet the formalities. So what was her PhD  
6:42
work? Well, we can take a look at her thesis.  Its title was Evolution of Galaxies and its  
6:47
Significance for Cosmology. In it, she makes  some of the first quantitative predictions of  
6:53
how galaxies will change over time by looking  at how the stars are evolving with time.
6:59
She showed that galaxy evolution  is something that can be observed  
7:04
and this was to grow into one of the  largest subfields within the study of  
7:08
galaxies. She looked at the process of  star formation and at how those stars  
7:14
would evolve and affect the recycling of  dust and gas in the interstellar medium.
7:19
This would shape the fate of the galaxy  itself and Beatrice was able to model this  
7:24
interconnectedness. Previous to Beatrice's work,  
7:28
it was thought that galaxies could be used as  standard candles to measure distances in space  
7:33
because they didn't change, but Beatrice  showed that galaxies could dim with age.
7:39
This had profound effects on how  astronomers came up with theories  
7:43
of the fate of the universe. Without this  insight, the leading theory had been that  
7:48
the universe would collapse in a big crunch.  Taking into account the changing nature of  
7:54
galaxies meant the data now looked more in  favor of the universe expanding forever.
8:00
Further observations 30 years later  using supernovae instead of galaxies  
8:05
as those standard candles were to show  that the expansion of the universe was  
8:09
in fact speeding up under the influence  of what astronomers call dark energy.  
8:16
Despite producing a great PhD in record time,  Beatrice felt deflated after this achievement.
8:22
She returned to Dallas with no job  prospects. She did apply for some  
8:26
grants to try and continue her research  from home and had short visiting stints at  
8:31
places like Caltech. She also adopted a second  child, Teresa. From all that I've read so far,  
8:37
it is clear that Beatrice loved her children  and did all she could to put them first.
8:42
It's also clear that these years post PhD were  a real struggle for her personally. When she'd  
8:48
moved to Dallas for her husband's job, it had  been with an understanding that it would only  
8:53
be temporary. But nearly ten years later, she was  still waiting for her turn to start her career.  
9:00
Everyone that met Beatrice could see her  potential and see how bright she was.
9:04
After a long time struggling, she knew  that getting a divorce from Brian would  
9:08
be the only way that she could shine. She  was offered an academic position at Yale  
9:13
and wanted to take the children with her,  but Brian didn't want her to. To avoid the  
9:18
children being fought over in court, she  gave way and moved to Yale on her own,  
9:23
continuing to visit and help with  child care arrangements when she could.
9:27
These aren't the kind of details I  usually mention too much in my videos,  
9:30
and a case of people splitting up and having  children live with one parent is an extremely  
9:35
common occurrence. In this case though, Beatrice  seems to have received quite a lot of criticism  
9:40
on the matter. Her daughter Teresa was later  quoted in a New York Times article saying that  
9:45
even though it was painful, she was proud that  her mom stood her ground and followed her career.
9:51
Moving to Yale, Beatrice finally got  to work on the questions that she had  
9:55
been inspired to answer as a child,  reading Hoyle's book about the origin  
9:59
of the universe. One of her papers was featured  in Time magazine, which is why she posed for this  
10:05
photo shoot at the Blackboard. She published over  100 papers, and looking through them, you can see  
10:11
topics like chemical evolution, abundance ratios,  metallicity distribution, and even dark matter.
10:18
These are all topics that make up the  modern field of galactic astronomy,  
10:22
and Beatrice was involved in all of them.  Her most impactful paper was published in  
10:27
1980 called The Evolution of Stars and Gas in  Galaxies. It received thousands of citations  
10:34
and its longevity is seen in the fact that  papers published this year are still citing it.
10:39
In it, Beatrice describes different  aspects of galactic evolution such as  
10:43
gaseous inflow and the composition of the  interstellar medium. She calls them pieces  
10:48
of a jigsaw puzzle that may someday be put  together. Another notable achievement of  
10:54
Beatrice's was that she organized a big  galaxy conference at Yale in 1977, which  
11:00
has been described as the single most important  galaxy conference in the history of the subject.
11:05
She also became Yale's first female professor  of astronomy. But at the height of her career,  
11:11
this story took a tragic turn. Just  a year after becoming a professor,  
11:15
she noticed a bleeding mole on  the back of her leg that she had  
11:19
previously ignored. She was diagnosed  with melanoma and underwent treatment.
11:23
During this time, she still kept busy and looked  after Teresa, who had come back to live with her.  
11:29
Beatrice continued to work throughout her illness,  
11:32
but over the course of a few years, became  very sick as treatment failed to save her.  
11:37
Her PhD students visited her bedside  and she helped them with their work.
11:41
She continued to work on her own research  too, and wrote her last paper from her bed  
11:46
in the Yale infirmary. She had to learn  to use her left hand in order to write  
11:50
it out. It was called Chemical Evolution  4, Some Revised General Equations. It was  
11:58
submitted 10 days before she died, in March  1981, and it was published after her death.
12:05
It includes calculations showing how to  separate living stars from dead remnants,  
12:10
and thus making models more consistent.
12:24
That building over there is where the astronomers  work today. And inside there's a small library  
12:29
with a bound copy of Beatrice's PhD thesis.  As an undergrad I got to stay there and  
12:34
meet Alan Gilmore and Pam Kilmartin,  who, using one of the telescopes here,  
12:39
discovered an asteroid in August 1981  that they named Beatrice Tinsley.
12:44
Beatrice's father, Edward Hill, called it a  kind of moving tombstone. There are some other  
12:49
small traces of her legacy across New Zealand,  like this street in Auckland named after her,  
12:55
and Mount Tinsley near Queenstown.  But still, many New Zealanders don't  
12:59
know about Beatrice, and her impact on  our understanding of the big questions.
13:03
Beatrice was friends with Vera Rubin, whose  work on galaxies provided key evidence for  
13:08
the existence of dark matter. I'd like to end  with Vera's words about Beatrice. She said,  
13:14
Even in her all too brief a life, Beatrice was one  of the giants of astronomy in the 20th century.  
13:20
There is no telling how much more we might have  learned if she had had a longer time to teach us.
13:26
While researching for this video, I saw that  Christine Catley's daughter, Nicola Scott,  
13:31
is currently driving an attempt to make a movie  about Beatrice, based on her mother's book. I  
13:36
hope this goes ahead, and that Beatrice's legacy  can continue to shine on. Thank you for watching,  
13:42
and thank you to my Patreon supporters  for making these videos possible.
13:46
A special shout out to today's  Patron cat of the day, Thorin.



2024/07/04

서울리뷰오브북스 [2024] -특집 리뷰: 믿음, 주술, 애니미즘

서울리뷰오브북스 (계간) : 14호 [2024] - 예스24
특집 리뷰: 믿음, 주술, 애니미즘



3/6이전 이미지 배너다음 이미지 배너

책소개
우리의 불가해한 믿음을 들여다보는 여섯 편의 전문 서평,
‘특집 리뷰’

《서울리뷰오브북스》의 새로운 코너 ‘고전의 강’

『경계를 넘는 공동체』부터 『혁명과 일상』까지,
서점가의 화제작들을 다루는 다채로운 ‘리뷰’

《서울리뷰오브북스》 2024년 여름호(14호)의 특집 주제는 ‘믿음, 주술, 애니미즘’이다. 우리는 무엇을, 왜, 어떻게 믿는가? 기성세대뿐 아니라 젊은 세대에게도 사주팔자와 신점이 인기이고, 디지털 시대에 걸맞게 전화와 스마트폰 메신저를 통해서도 ‘용한 곳’에 접속할 수 있다. 그러나 한편으로는 정치인이나 경영인이 ‘주술’에 의지한다는 혐의를 받으면 지지율과 주가가 요동친다. 무당·지관·장의사가 주인공으로 등장하는 영화 〈파묘〉(2024)가 오컬트 장르 최초로 천만 관객을 동원하는 동시에, OTT에서는 ‘사이비 종교’를 다룬 다큐멘터리가 공개되어 세간의 주목을 받고, 많은 이들의 분노와 경악을 자아냈다. 혹자는 근대로의 이행을 ‘탈주술화’ 과정이라 했지만, 2024년 한국 사회를 살아가는 우리는 여전히 주술과 함께 살아간다. 《서울리뷰오브북스》 14호에서는 이런 현실을 마주 보며 우리의 불가해한 믿음과 그 믿음의 대상들을 깊이 들여다보기 위해 종교학, 문화인류학, 과학학, 역사학, 자연과학 분야 전문가 6인이 머리를 맞댔다.

종교학자 한승훈은 이창익의 『미신의 연대기』를 리뷰하며 ‘미신’이란 무엇인지, 인간의 기괴한 믿음을 어떻게 마주할 것인지에 답한다. 권석준 편집위원은 과학적 회의주의자 마이클 셔머의 『왜 사람들은 이상한 것을 믿는가』를 통해 패턴 완성이 잘못된 믿음과 광신으로 이어지는 과정을 살펴본다. 무속 현장을 연구하고 있는 오성희는 두 여성 학자의 인류학적 무속 연구의 결과물인 『무당, 여성, 신령들』과 『한국 무교의 문화인류학』을 읽으며 한국 무속과 여성들 삶의 내면을 파악해 본다. 임종태(서울대 과학학과)는 지난 2월 작고한 ‘풍수 학인’ 고 최창조(1950-2024) 선생의 『한국의 풍수사상』을 다시 읽으며, 풍수라는 ‘전근대적’ 술수(術數)를 ‘현대적’ 학문으로 정립하고자 한 그의 여정을 좇는다. 심재훈(단국대 사학과)은 인신 공양과 식인 풍습이 만연했던 상나라의 흥망성쇠를 다룬 『상나라 정벌』을 비판적으로 독해한다. 홍성욱(본지 편집위원, 서울대 과학학과)은 애니미즘적 감수성의 복원을 주장하는 『애니미즘과 현대 세계』를 읽으며 과거와 다른 현대 사회의 ‘객체’들과의 관계성을 논의한다.

이번 호부터 《서울리뷰오브북스》는 새로운 코너 ‘고전의 강’을 통해 현재 우리에게 닥친 문제의 근본을 이해하기 위해 반드시 읽고 넘어가야 할 고전을 꼽고, 그 책을 오늘날의 시각에서 다시 살펴보는 작업을 시도한다. ‘고전의 강’이 탐독하는 첫 번째 주제는 ‘진화’이다. 오늘날 우리가 세상을 이해하는 데 가장 중요한 개념 중 하나인 진화는 찰스 다윈의 위대한 연구 이후, 다양한 맥락에서 이해되고 심화·발전되어 왔다. 진화심리학은 이런 지적 탐구가 낳은 한 결실이다. 정우현(본지 편집위원, 덕성여대 약학과)은 진화심리학을 이해하는 데 반드시 거쳐야 할 필독서이자 현대의 고전이라 할 로버트 라이트의 『도덕적 동물』을 읽으며, 유전과 도덕의 관계를 심층적으로 검토한다.

리뷰 코너에서는 유럽의 중심에서 중국을 이야기하는 인류학자 샹바오의 『경계를 넘는 공동체』부터, 영화라는 매체의 본성과 미적 가능성을 탐색하는 지그프리트 크라카우어의 『영화의 이론』과 질베르토 페레스의 『영화, 물질적 유령』, 북한에 대한 통설에 이의를 제기한 김수지의 『혁명과 일상』, 월북 지식인 김수경의 생애를 톺아보는 이타가키 류타의 『북으로 간 언어학자 김수경』 등, 서점가의 화제작들을 두루 다루었다.
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