Studying The Stars To Understand The Universe

EXPERT COMMENT: How we’re using the largest ever recorded set of galactic data to study the stars

Astrophysicist Dr Phil Sutton explains the possibilities opened up by new data from the European Space Agency’s Gaia satellite.

The Gaia satellite. After 22 months of observations, the second release of data contains the position and brightness of 1,692,919,135 stars

The Gaia mission is a space-based observational survey of over 1 billion stars in our local neighbourhood, the Milky Way (pictured above).It will measure the precise position of stars using a technique known as astrometry.

This will give a detailed three-dimensional map of the Milky Way and is complemented by spectroscopic measurements of the same stars.

Here, along with the precise position of stars in the Milky Way, the Doppler effect is used to find relative velocities of stars by a shift in wavelength of their observed light.

The result is a detailed kinematic map of stars in our local neighbourhood, which is important, as we still do not fully understand why stars move the way they do in galaxies.

Observations dating back to the 1930’s suggested that the rotation curves of galaxies do not fit with Keplerian orbits.

For planets and asteroids in the solar system, their orbits are generally well understood and follow Keplerian laws.

However, at a galactic scale, it was found that galaxies rotated far too fast for the matter we could see.

This discovery led to the concept of dark matter, which is needed to increase the orbital velocities of stars in galaxies.

Along with the increased orbital velocities, stars are also observed to exhibit some randomness to their motion around the centre of galaxies.

Obtaining a detailed kinematic map of our own galaxy can help us refine our current understanding of complicated dynamics within galaxies.

Future results from Gaia are likely to shape the future research of many astrophysicists.

For myself, I am currently looking at how the movement of the Sun, specifically the passage through the spiral arms, can affect the Earth.

This can be through enhanced Milankovitch cycles or gravitational scattering of solar system objects caused by close encounters with other nearby stars.

Much of our understanding of the universe comes from how we observe astronomical objects move relative to us and one another.

Therefore, creating the most detailed kinematic map of the Milky Way will help us appreciate objects we cannot see and physics we currently do not understand.

I also have an interest in gravitational waves and the types of objects that act as sources and other objects that we can use to detect their presence.

The main science goal of another space telescope survey Kepler was to find new planets around other stars.

It succeeded with now thousands of planets discovered and confirmed.

 

However, secondary to the main mission it also discovered many new types of variable stars, like the heartbeat star.

Due to the nature of the Gaia mission and its measurements various other secondary science is possible.

For example, the detection of certain frequencies of gravitational waves, help constrain the cosmological constant (the rate at which the universe is known to be expanding) and even survey a large number of asteroids in the solar system.

Gravitational waves are of interest to astrophysicists as they exist over a very broad range of wavelengths.

At some of the smallest scales, compact binary systems comprised of black holes or neutron stars or neutron stars can have wavelengths on the order of km, while gravitational waves from the early universe in the form of a polarisation of the Cosmic Microwave Background can wavelengths on the order of mega light-years (1,000,000 light years).

Detecting different wavelengths allows us to probe different physics and astronomical objects and get a better understanding of the universe we reside in.

 

The above article was written as part of a press release by Loughborough University. Original press release can be found here.

Historical First Astronomy Observation At University Of Lincoln

On the evening of 15th February Students studying physics at the University of Lincoln carried out their first observations of the night sky. This was the historical first practical astronomy session with the aim of expanding our practical element for you physics students. On the roof of the Isaac Newton Building students used a 8 inch (203mm) Schmidt-Cassegrain reflecting and 4.75inch (120mm) refracting telescope to view various interesting astronomical objects. Even in the centre of Lincoln we were able to clearly observe Orion’s nebula. A deep sky object which is a cloud of gas and dust illuminated by nearby young hot blue stars that have recently formed.

The plan is to loan out some of our telescopes to allow students to make their own observations in their own time.

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New top speed record for a car

Dr Phil Sutton

Yesterday saw the historic launch of SpaceX’s Falcon Heavy rocket with the non-traditional payload of a Tesla Roadster. At the beginning of the week the fastest cars are:

The fastest road car – Hennessey Venom GT with a top speed of 270+mph (434 kph).

The land speed record is currently just over 760 mph (1223 kph) by ThrustSSC.

Should note that this does not include cars that may have been dropped from planes reaching terminal velocity (order of ~100 mph / 160 kph) or those that have travelled on planes (~600 mph / 965 kph).

To put object into space and escape the gravity of Earth it must first overcome the escape velocity from the surface. Essentially this occurs when an objects kinetic energy becomes equal to the gravitational potential energy. For Earth this approximates to about 11.2 km/s. (40,300 kph). However, since a rocket…

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