ASPACE-Q 

The Astrophysics,  Space  Exploration and Quantum Computing Group   

 ASPACE-Q 

The Astrophysics,  Space  Exploration and Quantum Computing Group   

05.12.2024















                Image credit: Ben Yuen and Angela Demetriadou


In an article published in mid-November in Physical Review Letters, two researchers from the School of Physics and Astronomy at the University of Birmingham described a new way to characterize the properties of a photon in a given medium, simplifying the mathematics underlying the theory.


Because the properties of photons are heavily dependent on the environment  in which they propagate, the mathematics describing them is extremely complex and involves solving an enormous number of equations to obtain an answer.


The two authors found a way to simplify these calculations, and the formalism they developed made it possible to model the properties of a photon emitted from the surface of a nanoparticle (a particle with dimensions 1,000,000,000 times smaller than 1 meter), to describe its interactions with the emitting source, and to understand how the photon propagated away from the source.


Finally, it became possible, for the first time, to generate an image of a photon, which turned out to be a particle shaped like a lemon.


However, the authors emphasized that this shape is valid only for a photon generated under these specific conditions and that it changes completely in a different environment due to the photon's dual nature, as both particle and wave. Thus, the wave stretches or shrinks, bends, slows down—in other words, it takes on a different shape depending on the environment through which it propagates, much like a dancer adapting their movements and body shape to the stage and the music they are performing to.


And, as the saying goes, “when life gives you (photon)-lemons…” 😊. The formalism developed by the team of researchers from Birmingham opens up a new universe of possibilities for photon exploitation: new ways of capturing light and developing innovative photovoltaic devices, a better understanding of photosynthesis and the creation of artificial photosynthesis, quantum communication, and many other applications yet to be imagined.

21.11.2024

Researchers from Durham University have developed a model to estimate the chances of intelligent life emerging in different universes, focusing on the effects of dark energy and star formation rates. 

Despite its name, the dark energy is not actually as “dark” as it sounds :) It is only called like this because we can not actually “see” it and know how it works, yet we do know that it represeents that one secret ingredient needed for explaining the accelerated expansion of the Universe. 

The article published in Monthly Notices of the Royal Astronomical Society highlights how our universe’s conditions for life may be rare, yet similar life-friendly conditions might exist even in universes with higher dark energy densities. This work updates theories like the Drake Equation, combining simulations and theoretical frameworks to explore the delicate balance required for life. 

 

‍                    The Drake Equation

 

According to the Royal Astronomical Society, the equation dr. Drake came up with could give a rough estimation of  “detectable extraterrestrial civilizations in our Milky Way galaxy”.  In order to do so, the formula takes into account the number of stars that are freshly born in the Milky Way each year,  how many stars have planets orbit them as well as the number of worlds that have the potential of supporting life.

 

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Compared to the initial equation, the newly developed model also considers the effect of dark energy density.

Terms of Drake equation explained

Credit: https://ras.ac.uk

How the same region of the Universe would look in terms of the amount of stars for different values of the dark energy density. Clockwise, from top left, no dark energy, same dark energy density as in our Universe, 30 and 10 times the dark energy density in our Universe. The images are generated from a suite of cosmological simulations.

Credit: Oscar Veenema

15.11.2024

In August 2024, scientists observed a small "minimoon" named 2024 PT caught briefly in Earth’s gravity. This space rock, about the size of a car, was spotted by the Hawaiian telescope ATLAS and will stay in Earth’s orbit only temporarily. Researchers are curious about its origins, as it could be a piece of an asteroid or even lunar debris. Studying these minimoons helps scientists better understand the nature and origins of such small, passing objects near Earth.


For more details, check put the article here!


Top left panel: a median combination stack of 11 x 75 s g filter images of 2024 PT5. An arrow indicating the width of 10″ is shown for scale, and the cardinal directions are indicated. Top right panel: a median combination stack of 5 x 50 s r filter images of 2024 PT5. Bottom left panel: a median combination stack of 2 x 60 s i filter images of 2024 PT5. Bottom right panel: a median combination stack of 2 x 60 s Z filter images of 2024 PT5. The image scale and cardinal in the r, i, and Z stacks are the same as in the g image stack.
Panel a: The first of four o-band ATLAS-Sutherland telescope discovery images of 2024 PT5 from 2024 August 7 21:11:57 UTC. The asteroid moved at a rate of 34.3 arcminutes per hour (13.7 degrees per day) in the northwest direction. The asteroid makes a  ∼ 9 pixel trail in the 30 s ATLAS exposures, indicated by the red circle. Panel b: the same as panel a but shows the image after subtracting static sources. Despite the presence of nearby stars, the asteroid is detected cleanly in the subtracted images. Panel c: the same as panel a, but the second of four o-band images containing 2024 PT5 taken on 2024 August 7 21:16:35 UTC. Panel d: the same as panel c but shows the image after subtracting static sources. The asteroid was detected with an apparent magnitude of o=17.13 in panel b and o=16.99 in panel c. The large black areas in the subtracted images are regions of saturated pixels from bright stars. The direction of the asteroid and cardinal directions are indicated in each figure.
ide view of the Earth co-rotating frame orbital trajectory of 2024 PT5 as it enters and leaves the Earth-Moon system between 2024 June and 2025 April in Cartesian Earth-Moon barycentric x and z coordinates. The daily position of 2024 PT5 is represented as blue points except the portion of its trajectory when it had  e g < 1 plotted in red. The position of the Earth is plotted with a cyan circle. The circular green-shaded region indicates the Hill sphere of Earth. The position of 2024 PT5 , when it was discovered, is marked by a green circle, and the position of 2024 PT5 when Gemini observed it is marked with a green X. A blue arrow indicates the direction of motion of 2024 PT5 along its orbital path.

Credit: Bolin, B. et al, preprint arxiv The discovery and characterization of minimoon 2024 PT5

Credits: ESA/ROB

01.11.2024

The European Space Agency (ESA), along with researchers and engineers from the 14 member states of the PROBA-3 Space Mission consortium, are preparing to receive the most beautiful Christmas gift: the launch of the mission, scheduled for December of this year. Romania is one of the 14 states and has contributed to both the development of hardware components (through IMT and COMOTI) and scientific contributions through AIRA who also developed the catalog tools and ISS who contributed in the early stages of the mission).

PROBA-3 consists of two satellites carrying three instruments for observing the Sun: ASPIICS (the main instrument for observing the solar corona, managed by the Royal Observatory of Belgium), DARA (an instrument measuring the total solar energy, essential for Earth's climate studies, developed by the Physical Meteorological Observatory in Switzerland), and the 3D Energetic Electron Spectrometer, developed by the Catholic University of Louvain, Belgium, an important tool for space weather studies.

The satellites will fly in formation with millimetre precision, unprecedented for space vehicles. 

The PROBA-3 satellites are tasked with creating an artificial solar eclipse in space, which will be repeated approximately 50 times a year and will last up to 6 hours during each rotation of the formation around the Earth. This will enable the observation of regions of the Sun that have not been sufficiently explored by researchers until now. Specialised solar observation instruments, such as the state-of-the-art ASPIICS coronagraph, will then be used to study phenomena occurring in the solar corona, such as coronal mass ejections, which are eruptions and explosions of plasma from the Sun. Observing these is important to better understand why the solar corona is so hot (around 1 million degrees Celsius), much hotter than the surface of the Sun (5,500 degrees Celsius). The temperature of the solar corona remains a mystery for researchers.

Another important phenomenon to study is the solar wind, the constant stream of charged particles emitted by the Sun, which dictates the space weather near Earth and can affect technology and communications on Earth.

Last but not least, this mission has led to significant technological advancements for space missions studying the Sun and beyond, using a new generation of sensors, advanced hardware components, and improved onboard software.

The PROBA-3 mission, which will simulate solar eclipses, is scheduled to leave Europe on November 1st, heading to its launch site in India. The two satellites will be transported to ISRO's Satish Dhawan Space Centre, located near Chennai.

For more information you can access the official page of the mission and the official announcement from ESA.

Stay tuned for updates on this exciting December launch!

01.02.2024

LISA HAS BEEN ADOPTED!


 

2024 kicked off in the best possible way as ESA announced the adoption of its largest space mission: LISA, the Laser Interferometer Space Antenna.


After more than 100 years since Einstein’s theory of relativity predicted the existence of gravitational waves, we are finally ready to listen to the sound of the Universe directly from space. LISA  is expected to be launched in the mid 2030’s and, according to ESA, the collaboration got to the point where it can actually start building all the needed components, stage also known as the “implementation phase”. All the details regarding the mission and the next steps are available on the official website.

Contact us at:

 iss dash sci at spacescience dot ro