Measuring the Sizes of Distant Stars
Scientists use intensity interferometry to measure star sizes with advanced telescopes.
Naomi Vogel, Andreas Zmija, Frederik Wohlleben, Gisela Anton, Alison Mitchell, Adrian Zink, Stefan Funk
― 6 min read
Table of Contents
Have you ever wondered how we can measure the sizes of stars that are light-years away? Well, scientists have come up with a clever trick called Intensity Interferometry. This method has been making waves in the field of astronomy and has recently been applied to some impressive Telescopes like H.E.S.S., MAGIC, and VERITAS. These fancy names sound like they belong in a superhero movie, but they are actually powerful telescopes designed to observe cosmic phenomena.
This article will take you through an exciting journey of how scientists used intensity interferometry to measure the sizes of stars. Let’s dive into the details without drowning in complex terminology!
The Basics of Intensity Interferometry
Intensity interferometry is not a new idea. It was first used in the 1960s by two clever chaps, Robert Brown and Richard Q. Twiss. They created a device called the Narrabri Stellar Intensity Interferometer, which managed to measure the sizes of several stars. However, the technique was put on the back burner for a while because technology didn’t keep up with the demands of this method.
Fast forward a few decades, and here we are! With advancements in tech, intensity interferometry has resurged and is being used to measure stars with impressive accuracy. This technique allows us to measure the light from stars using separated telescopes, and it takes advantage of how light waves behave when they are in sync.
How It Works
Imagine you are at a concert, and you hear a favorite song playing. If you close your eyes and listen closely, you can hear the sounds coming from all around you. The same idea applies here. When light waves from a star travel to two different telescopes, they can be combined to create a pattern that helps scientists figure out the star's characteristics.
The trick lies in observing how the light waves from a star interact with each other. By Measuring the intensity of these light waves, scientists can determine the star's size, even from vast distances. It’s like putting together a jigsaw puzzle, where every piece gives you a clearer picture of the whole.
The Current Campaign
In 2022, scientists took their first shot at intensity interferometry with the H.E.S.S. telescopes situated in Namibia. It was like a camping trip, but instead of roasting marshmallows, they were armed with high-tech equipment to measure the sizes of stars. They had some success, measuring the angular diameter of two stars.
However, they wanted more! So, in 2023, they upgraded their setup for a second campaign. This time, they aimed to perform simultaneous measurements in two different colors of light. It’s like trying to capture a rainbow while making sure you don’t miss any colors!
New and Improved Setup
The 2023 campaign introduced a third telescope to the team, allowing for even more Data collection. Each telescope had extra filters to focus on two different wavelengths of light. This means they could gather information about the stars using different colors, adding a layer of detail to their measurements.
Before the campaign started, the scientists had to prepare everything meticulously. This included a lot of adjustments and calibrations, ensuring that the equipment would work perfectly on the night of observation. It’s like trying to bake a soufflé – one wrong move can ruin the whole thing!
Targeting Stars
During the campaign, the scientists set their sights on four stars: Mimosa, Eta Centauri, Nunki, and Dschubba. These stars were chosen based on their brightness and how well they could be observed. Think of it as picking the best players for your fantasy football team!
The team tracked these stars as they moved across the sky, making sure to gather as much data as possible. The measurements took place during a time when the moon was bright, and the telescopes were unable to observe gamma rays. So, instead of wasting the perfect opportunity, they turned their attention to the stars!
Data Collection and Analysis
Once the measuring began, it was a matter of gathering data and analyzing it. Each measurement was carefully recorded, and the data was cleaned up to ensure accuracy. This process is vital because, without precise data, the results would be about as useful as a chocolate teapot.
After the data was collected, the scientists could finally look at the results. They wanted to understand the angular sizes of the stars they observed, using both simple and more complex models to analyze them. It was like comparing apple pie to a five-layer chocolate cake – both are delicious, but they require different recipes!
Results of the Observations
When the dust settled, the scientists had some exciting findings. The measurements showed that the sizes of some stars varied based on the wavelengths of light they used. In simple terms, the measurements were consistent with what they’d hoped to find, but some stars had a surprise twist – their sizes changed depending on the color of light!
For instance, Mimosa and Eta Centauri had similar results for both colors, making it like comparing two best friends who wear matching outfits. But for stars like Nunki and Dschubba, the differences were significant. This led to some head-scratching moments as scientists tried to understand why these stars didn’t behave like their peers.
Tackling Challenges
The scientists encountered some challenges along the way. One notable hurdle was the issue of misalignment in the telescopes. Sometimes, the telescopes didn’t point precisely at the stars. It's like trying to take a selfie with your friends but not getting everyone’s face in the frame.
To address this, the team made adjustments during the measurements, ensuring they captured the photonic equivalent of their subjects' "good side." While it took some teamwork and quick thinking, they managed to collect the necessary data to continue their analysis.
Looking Ahead
The scientists are excited about the future. They plan to equip all four H.E.S.S. telescopes with this high-tech setup, allowing for even better measurements. This means they will be able to create a more detailed map of the stars they observe, capturing even the faintest ones.
They’re also looking to take on fainter stars and binary star systems. This is like going from playing in the local league to joining a professional team – it’s a big leap that promises thrilling results!
Conclusion
To sum it all up, the 2023 intensity interferometry campaign was a success, showcasing how advanced telescope technology can help measure the sizes of stars in ways we never thought possible. The scientists managed to confirm their findings while uncovering new mysteries about some stars behaving unlike their peers.
This work not only adds to our understanding of the universe but also shows how two colors of light can help uncover deeper insights. Despite the challenges faced along the way, the team came out on top, ready to continue their starry-eyed adventure!
So, next time you look up at the night sky, remember that we’re not just gazing at twinkling lights; we’re peering into a world of science, technology, and wonder that keeps us questioning and exploring the universe far beyond what our eyes can see.
Title: Simultaneous Two Colour Intensity Interferometry with H.E.S.S
Abstract: In recent years, intensity interferometry has been successfully applied to the Imaging Atmospheric Cherenkov Telescopes H.E.S.S. , MAGIC, and VERITAS. All three telescope systems have proven the feasibility and capability of this method. After our first campaign in 2022, when two of the H.E.S.S. telescopes in Namibia were equipped with our external setup and the angular diameter of two stars was measured, our setup was upgraded for a second campaign in 2023, where the goal is to perform simultaneous two colour measurements. The second campaign not only involves a third equipped telescope, but also each mechanical setup now includes two interference filters at two different wavelengths (375 nm and 470 nm) with a broader bandwidth of 10 nm. This enables having simultaneous two colour measurements, which yields information about the star's physical size at different wavelengths. This is the first time that simultaneous dual-waveband intensity interferometry measurements are performed. The angular diameter results of the 4 stars, Mimosa (beta Cru), Eta Centauri (eta Cen), Nunki (sigma Sgr) and Dschubba (delta Sco), are reported, where the effects of limb darkening are also taken into account.
Authors: Naomi Vogel, Andreas Zmija, Frederik Wohlleben, Gisela Anton, Alison Mitchell, Adrian Zink, Stefan Funk
Last Update: 2024-11-25 00:00:00
Language: English
Source URL: https://arxiv.org/abs/2411.16471
Source PDF: https://arxiv.org/pdf/2411.16471
Licence: https://creativecommons.org/licenses/by/4.0/
Changes: This summary was created with assistance from AI and may have inaccuracies. For accurate information, please refer to the original source documents linked here.
Thank you to arxiv for use of its open access interoperability.