New Horizons Images Enable First Test of Interstellar Navigation

Illustration of NASA’s New Horizons spacecraft navigating the outer solar system.

Joe Olmsted/STScI

After departing from our solar system, NASA’s New Horizons spacecraft finds itself considerably distant from Earth, causing the stars of the Milky Way to appear in notably different positions compared to our terrestrial views. Astronomers are harnessing this altered perspective to determine the location of galaxy probes, marking the first instance of intergalactic navigation.

Launched in 2006, New Horizons initially observed Pluto before continuing beyond, traversing the Kuiper Belt—an immensely expansive region of rocky debris and dust billions of miles from the Sun. Currently, the spacecraft is hurtling through space at tens of thousands of kilometers per hour.

When gazing at the night sky from Earth, stars seem widely spread apart, so unless equipped with a strong telescope, their positions appear constant from various locations. In contrast, the New Horizons perspective reveals a significant shift in star positions due to the parallax effect. This phenomenon was demonstrated in 2020 when the probe captured images of two nearby stars, Proxima Centauri and Wolf 359.

Now, Todd Lauer from the U.S. National Institute of Light Change Astronomy in Arizona and his team have utilized this effect to gain a new perspective. They accomplished this by comparing images of Proxima Centauri and Wolf 359 taken by the probe with measurements from the Gaia Space Telescope.

“There’s a three-dimensional map of the galaxies around us, allowing you to see your position,” says Lauer. “Using your own camera on a spacecraft offers incredible accuracy.”

To determine the spacecraft’s location, Lauer and his team analyzed the star positions detected by the New Horizons camera, tracing their lines back to the closest intersection point. They then referenced the precise locations of both stars from the Gaia star map to ascertain this point’s relation to the solar system.

This two-frame animation illustrates the changing position of Proxima Centauri as observed from Earth and New Horizons.

Nearly every spacecraft utilizes NASA’s Deep Space Network (DSN) to determine its position within a margin of tens of meters through a network of radio transmitters on Earth. In contrast, the parallax method provides a less precise estimation, determining New Horizons’ location within a 6,000-kilometer sphere, roughly half the distance from Earth to the Sun.

“We don’t aim to replace the Deep Space Network; this is merely a proof-of-concept demonstration,” Lauer notes. Yet, advancements in cameras and equipment could enhance accuracy by up to 100 times.

Employing this technique for interstellar navigation could yield superior location accuracy compared to the DSN. This not only facilitates the spacecraft’s journey further from Earth but also provides more reliable location tracking, enabling autonomous operations without relying on radio signals from the solar system. Massimiliano Vasile from Strathclyde University in the UK emphasizes this potential.

“When we venture to real stars, we’re talking about light-years,” Vasile explains. “The signal from the Deep Space Network must traverse all the way there, moving at light speed, taking years to reach its destination.”

However, Vasile points out that no agency currently has a mission aimed at deeper exploration of interstellar space, limiting the immediate utility of this technique.

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Source: www.newscientist.com

Hubble Space Telescope and New Horizons team up to study Uranus

In a new study, astronomers compared high-resolution images of Uranus from the NASA/ESA Hubble Space Telescope with more distant views from NASA’s New Horizons spacecraft. Their results could serve as “ground truth” observations to use as a baseline for interpreting exoplanet direct imaging data from future observatories.

In this image, two three-dimensional shapes of Uranus (top) are compared to the actual views of Uranus from Hubble (bottom left) and New Horizons (bottom right). Image credits: NASA/ESA/STScI/Samantha Hasler, MIT/Amy Simon, NASA-GSFC/New Horizons Planetary Science Theme Team/Joseph DePasquale, STScI/Joseph Olmsted, STScI.

Direct imaging of exoplanets is an important technique for understanding their potential habitability and provides new clues to the origin and formation of our own solar system.

Astronomers use both direct imaging and spectroscopy to collect light from observed planets and compare their brightness at different wavelengths.

However, exoplanets are notoriously difficult to image because they are so far away.

Their images are just pinpoints, so they aren’t as detailed as our close-up view of the world around the sun.

Astronomers can also directly image exoplanets only in “partial phase,” when only part of the planet is illuminated by its star as seen from Earth.

Uranus was an ideal target as a test to understand future long-range observations of exoplanets by other telescopes for several reasons.

First, many known exoplanets are gas giants with similar properties. Also, at the time of the observation, New Horizons was on the far side of Uranus, 10.5 billion kilometers (6.5 billion miles) away, and was able to study the twilight crescent moon. This is not possible from Earth.

At that distance, New Horizons’ view of the planet was just a few pixels wide of its color camera (Multispectral Visible Imaging Camera).

Meanwhile, Hubble’s high resolution allowed it to see atmospheric features such as clouds and storms on the dayside of the gas world from its low orbit, 2.7 billion kilometers (1.7 billion miles) from Uranus. .

Samantha Hassler, an astronomer at the Massachusetts Institute of Technology, said: “We expected Uranus to look different depending on the observation filter, but New Horizons data taken from different perspectives actually show that Uranus looks different than expected.'' It turned out to be much darker than that.”

The gas giant planets in our solar system have dynamic and variable atmospheres with changing cloud cover. How common is this in exoplanets?

Knowing the details of what Uranus’ clouds looked like from Hubble will allow researchers to test what they can interpret from New Horizons’ data.

In the case of Uranus, both Hubble and New Horizons observed that the brightness does not change as the planet rotates. This indicates that the cloud characteristics are not changing due to the rotation of the planet.

But the significance of New Horizons’ detection has to do with how the planet reflects light at a different phase than what Hubble and other observatories on or near Earth can see.

New Horizons showed that exoplanets can be dimmer than predicted at partial and high phase angles, and that their atmospheres reflect light differently at partial phase.

“The groundbreaking New Horizons study of Uranus from a vantage point that cannot be observed by any other means adds to the mission’s treasure trove of new scientific knowledge and, like many other data sets obtained on the mission, will Dr. Alan Stern, Principal Investigator of New Horizons and Research Scientist at the Southwest Research Institute, said:

“NASA’s next Nancy Grace Roman Space Telescope, scheduled to launch by 2027, will use a coronagraph to block out starlight and directly observe gas giant exoplanets,” Hassler said. Ta.

“NASA’s Habitable World Observatory, in its early planning stages, will be the first telescope specifically designed to search for biosignatures in the atmospheres of rocky Earth-sized planets orbiting other stars. .”

“Studying how known benchmarks like Uranus appear in distant images will help us have more solid expectations as we prepare for these future missions. And it will help our It’s critical to success.”

Scientists are result this week’s DPS56Annual Meeting of the Planetary Science Division of the American Astronomical Society.

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S. Hassler others. 2024. Observations of Uranus at high phase angles by New Horizons Ralph/MVIC. DPS56

This article has been adapted from the original release by NASA.

Source: www.sci.news