AstroBlonde


Here you can follow my studies in
Astrophysics and read all other useless
stuff that goes on in my life...

Are you interested in astronomy?

The last couple of days I've been sick. That has given me more time to update my homepage, AstronomiGuiden.


Screen print from AstronomiGuiden today


I've been asked some questions about a planet made of diamonds, that has an orbit around a neutron star. I can't say I know much about that planet, but I suspect it's an old star which has "died", leaving carbon and oxygen behind. Because of the last stages in a star's life, the core is belived to shrink and the density can get higher. From Wikipedia:

"In mineralogy, diamond is an allotrope of carbon, where the carbon atoms are arranged in a variation of the face-centered cubic crystal structure called a diamond lattice."

"Most natural diamonds are formed at high-pressure high-temperature conditions existing at depths of 140 to 190 kilometers (87 to 120 mi) in the Earth mantle."

So, my guess is that it's a dead star orbiting the neutron star. All gas might have been stolen by the neutron star as well. But, this is only what I think it might be.

For all you Swedes, you can read about this at Aftonbladet. I don't think Aftonbladet is especially good when it comes to science, but here's the link anyway:
Ny diamantplanet upptäckt
Scientific american has written about it here:
Diamond World Discovered by Astronomers

Something else that might be interesting is that Caffau et al. (Nature, today’s issue) report that a "mysterious" star has been discovered. Apparently a star in the Milkyway with very low metalicity, ie. low abundence in heavy elements. That means that the star contains almost exclusively of Hydrogen (H) and Helium (He). Those kind of stars are believed to be very old stars, because heavier elements are belived to form when stars dies.

Let's take it from the start:
It is belived that the Universe, when it was young, contained only light elements such as Hydrogen (H), Helium (He), Lithium (Li) and Beryllium (Be). But today, we have other heavier elements such as Iron (Fe) and lots of others. So, how was those elements created? Well, the most likely thing that can create heavier elements are stars. When stars die, they can explode and send a lot of gas out in the Universe. That gas, can then create new stars, but those new stars will contain of heavier elements than the star before. This leads to heavier and heavier elements for every generation of stars.

When knowing this, you can perhaps see why this star is different. It seems like it doesn't have heavier elements. That's why people are saying that it might be a really old star, perhaps the oldest one we've found so far. It is also located withing our galaxy, which contains a lot of gas. So, this is a new, interesting discovery! What else that is interesting is that this will be a new challenge for astronomers to understand. Earlier models for how stars are formed need some heavier elements to contribute to its formation. So this star should not have been formed according to the understanding we have so far. Very interesting indeed!

Swedish links:
ESO Swedish - Stjärnan som inte borde finnas
Sveriges radio - Mystisk stjärna funnen i Vintergatan

English link:
ESO English - The Star That Should Not Exist

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Courses I've studied at Uppsala University

Math
Introduction to Mathematics 3 points
Algebra MN1 7,5 points
Analysis MN1 15 points
Linear Algebra MN1 7,5 points
Analysis MN2 15 points
Fourier Analysis with Applications 7,5 points
----------------------------------------------------
Math total: 55,5 points (60 points = 1 year)

Computing
Use of MATLAB 7,5 points
Scientific Computing NV1 7,5 points
----------------------------------------------------
Computing total: 15,0 points (60 points = 1 year)

Physics
Science in Society MN1 7,5 points
Quantum Physics and Astrophysics 9 points
Mechanics MN1 7,5 points
Mechanics MN2 7,5 points
Wave Physics NV1 7,5 points
Mathematical Methods of Physics NV1 7,5 points
Electromagnetism MN1 7,5 points
Solid State Physics MN1 7,5 point
Thermodynamics MN1 7,5 points
Statistical Mechanics MN1 7,5 points
Theory of Special Relativity 4,5 points
Quantum Mechanics MN1 7,5 points
Electromagnetic field theory MN1 7,5 points
----------------------------------------------------
Physics total: 96,0 points (60 points = 1 year)

Astrophysics
The structure of the Universe 7,5 points
Introduction to Astronomy 7,5 points
Principles of Astronomy MN1 7,5 points
Astrophysics II 5 points
Physics of the Planetary System 10 points
Radiation processes in Astrophysics 10 points
Galaxies 10 points
Cosmology 10 points
Dynamical processes in astrophysics 10 points
Celestial Mechanics 5 points
Observational Astrophysics I 5 points
Observational Astrophysics II 10 points
----------------------------------------------------
Astrophysics total: 97,5 points (60 points = 1 year)

Thesis
Image reduction and dust map construction of the local galaxy UGC08012 by using NOT observations
bryt
About Uppsala University

Uppsala University (Swedish: Uppsala Universitet) is a research university in Uppsala, Sweden. Founded as early as 1477, it is the oldest such institution in the Nordic countries, and for centuries has been one of Europe's most renowned seats of learning.

One of the main centres of higher education in Europe, the university rose to pronounced significance during the rise of Sweden as a Great Power at the end of the 16th century and was then given a relative financial stability with the large donation of King Gustavus Adolphus in the early 17th century. Uppsala also has an important historical place in Swedish national culture, identity and for the Swedish establishment: in historiography, literature, politics, and music. Many aspects of Swedish academic culture in general, such as the white student cap, originated in Uppsala. It shares some peculiarities, such as the student nation system, with Lund University and the University of Helsinki.

Uppsala belongs to the Coimbra Group of European universities. The university has nine faculties distributed over three 'disciplinary domains'. It has about 40,000 students (20 000 full-time eq.), and about 2,000 doctoral students. It has a teaching staff of 4,000 (part-time and full-time) out of a total of 6,000 employees. Of its annual turnover of around 4.3 billion SEK (approx. 715 million USD), approximately 60% goes to graduate studies and research.

Architecturally, Uppsala University has traditionally had a strong presence in the area around the cathedral on the western side of the River Fyris. Despite some more contemporary building developments further away from the centre, Uppsala's historic centre continues to be dominated by the presence of the university.

Source: Wikipedia

Newspapers I've been in

Newspaper: Populär Astronomi, Sep 2009, No 3, Year 10, Page 22
Language: Swedish
About: My homepage, my education and astronomy interest, and me moving to Australia.
Pages: 4

Newspaper: Upsala Nya Tidning, Dec 7 2008, B6
Language: Swedish
About: My homepage and my astronomy interest
Pages: 4
bryt

Articles I've written

Popular scientific
Newspaper: Populär Astronomi, Sep 2009, No 3, Year 10, Page 30
Language: Swedish
Swedish title: Behövs verkligen mörk materia?
English title: Do we really need dark matter?
About: The MOND theory.
Pages: 4

Popular scientific
Newspaper: Populär Astronomi, Sep 2008, No 3, Year 9, Page 32
Language: Swedish
Swedish title: Solens nya innehållslista
English title: The Sun's new content list
About: The chemical abundances in the Sun according to Martin Asplund et al.
Pages: 4

About this blog

My name is Åsa, 30 years old and I was born in Uppsala, Sweden. The last couple of years I've been studying math, physics and astrophysics at Uppsala University, Sweden.

On this blog you can follow my work to finish my master's degree as well as other private things going on in my life.

I'm currently in: Uppsala, Sweden.

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