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NASAScienceTech

NASA’s tiny “artificial star” to launch in 2029

By 2029, NASA aims to launch its first "artificial star" into orbit as a cosmic calibrator, with potential to unlock secrets of exoplanets and the universe's expansion.

By
Shubham Sawarkar
Shubham Sawarkar's avatar
ByShubham Sawarkar
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I’m a tech enthusiast who loves exploring gadgets, trends, and innovations. With certifications in CISCO Routing & Switching and Windows Server Administration, I bring a sharp...
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Jun 19, 2024, 8:30 AM EDT
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Space. 17th May, 2024. This NASA Hubble Space Telescope image captures a triple-star star system. Looking like a glittering cosmic geode, a trio of dazzling stars blaze from the hollowed-out cavity of a reflection nebula in this new image from NASA's Hubble Space Telescope. The triple-star system is made up of the variable star HP Tau, HP Tau G2, and HP Tau G3. HP Tau is known as a T Tauri star, a type of young variable star that hasn't begun nuclear fusion yet but is beginning to evolve into a hydrogen-fueled star similar to our Sun. T Tauri stars tend to be younger than 10 million years old.
Photo: Alamy
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For astronomers, the universe is a playground of giants – colossal telescopes peering into the abyss, galaxies swirling with billions of stars, and behemoth stars exploding in spectacular supernovas. But a new and revolutionary tool is about to join the cosmic crew: a miniature satellite, no bigger than a breadbox, that will act as an “artificial star.”

This may sound like something out of science fiction, but NASA‘s recently approved Landolt Space Mission is a game-changer for astronomical research. Costing a mere $19.5 million, this tiny satellite promises to unlock a treasure trove of knowledge about our universe, helping us understand everything from the nature of exoplanets to the expansion rate of the cosmos itself.

The secret lies in the satellite’s very nature. Unlike real stars, whose light output remains a bit of a mystery, Landolt will be a precisely calibrated beacon. This CubeSat, named after the late astronomer Arlo Landolt, will fire lasers with a specific number of light particles, allowing astronomers to fine-tune their telescopes for accurate light measurement.

Traditionally, astronomers rely on real stars for calibration, but this approach has limitations. Firstly, the exact brightness of a distant star is anyone’s guess. Secondly, Earth’s atmosphere acts like a cosmic dimmer switch, absorbing starlight and introducing errors in measurements. Landolt eliminates these problems. By providing a known and steady light source, it becomes the ultimate ruler for astronomers, enabling them to measure the light emitted from other celestial objects with ten times the current accuracy.

Imagine a 1000-piece jigsaw puzzle with half the pieces missing. Landolt is like finding those missing pieces, providing crucial details that were previously hidden. As astronomer Tyler Richey-Yowell explains, “All of our astronomy is based on light… We really need to know how much light we are actually receiving.”

This precise light measurement unlocks a treasure chest of information. From a single ray of light, astronomers can glean a star’s temperature, mass, and even the potential for harboring life-supporting exoplanets. Knowing a star’s temperature is key to pinpointing the habitable zone, the region around the star where a planet could potentially have liquid water on its surface – a crucial ingredient for life as we know it.

Landolt’s applications extend far beyond exoplanet hunting. Astronomers can use it to measure light from exploding stars (supernovae), which plays a vital role in calculating the expansion rate of the universe. Currently, cosmologists face a frustrating paradox – different methods yield slightly different values for the universe’s expansion rate. Understanding this expansion rate is crucial for unraveling the mysteries of dark energy, the invisible force pushing galaxies apart.

In essence, Landolt, this tiny space tool, has the potential to revolutionize our understanding of everything from the tiniest exoplanets to the vast expanse of the universe. As Richey-Yowell says, “It really will be revolutionary for astronomy.” With its launch slated for 2029, the scientific community eagerly awaits this new era of precise and powerful astronomical observation.


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