Connect with us

Published

7 months ago

on

Voyager 1, the farthest human-made object from Earth, has recently undergone a critical adjustment to its thruster system as it navigates the vast expanse of interstellar space. Despite being operational for 47 years, the spacecraft required a clever fix to maintain its alignment and continue sending valuable data back to Earth.

Voyager 1’s Thruster Issue

Voyager 1, launched in 1977, faced difficulties with its thrusters, which are essential for keeping the spacecraft oriented correctly. The problem stemmed from a fuel tube clogging issue, a known problem that has affected the spacecraft for over two decades. The ageing spacecraft, which relies on a dwindling power supply, needed a strategic switch to a different set of thrusters to avoid potential communication loss.

The Complex Fix

Due to the spacecraft’s advanced age and diminished power, engineers at NASA’s Jet Propulsion Laboratory (JPL) had to approach the problem with extra caution. The team decided to repurpose one of Voyager 1’s attitude thruster branches, which had been inactive due to severe cold and power constraints.

To address this, they briefly activated a heater to warm the thruster before switching it on. This manoeuvre was critical to ensure the spacecraft remained properly oriented and capable of relaying data.

Voyager’s Ongoing Mission

Voyager 1, along with its twin Voyager 2, was originally launched to explore the outer reaches of the solar system. Over time, both spacecraft have provided invaluable information about distant planets and the space beyond our solar system. Despite the technical hurdles, Voyager 1 continues to send data and is expected to remain operational through at least the 50th anniversary of its mission in 2027.

Future Prospects

Engineers at JPL are committed to maintaining the spacecraft’s functionality as long as possible. The recent adjustments demonstrate the ongoing ingenuity required to manage and extend the life of these historic missions. As Voyager 1 ventures further into interstellar space, its ability to adapt to new challenges will continue to be proof of the longevity and resilience of human space exploration.

Related Topics:
Continue Reading

Science

Astronomers Detect Methane in the Atmosphere of the Nearest T Dwarf Star to Earth

Published

3 days ago

on

April 12, 2025

By

Astronomers Detect Methane in the Atmosphere of the Nearest T Dwarf Star to Earth

The scientists have found methane in the atmosphere of WISEA J181006.18 −101000.5, the T dwarf closest to Earth. The study was published in the online preprint journal arXiv on March 28, and the final, revised version was published on November 17. The WISE1810 is a metal-poor T dwarf planet, which is situated at a distance of 29 light years from the Earth. The effective temperature of the dwarf is reported to be within the range of 800–1,300 K.

Methane Signature Surprises Astronomers

According to a Phys.org report, the finding is made greatly possible by the present 10.4-m Gran Telescopio Canarias (GTC). The detection of methane in the atmosphere of the dwarf planet has further made its classification as T-type instead of L-type, which was earlier suggested in previous studies, the publication notes. The study further reveal that there are no traces of carbon monoxide and potassium in the atmosphere of the WISE1810. 

The study further highlights that the carbon abundance in the planet is estimated to be -1.5 dex, while the effective temperature could be around 1,000 K. The author of the paper further revealed that the low metallicity of the T dwarf planet could be due to the non-detection of atomic potassium. However, a lower temperature could also boost this effect, the report further highlights. The study also found that WISE1810 has a heliocentric velocity of -83 km/s. 

The 10.4-m Gran Telescopio Canarias (GTC) supplies a significant contribution to finishing WISEA J181006.18−101000 observations. Interestingly, the previous observations of the dwarf platent suggested that the atmosphere of the dwarf planet was dominated by hydrogen and water vapour. Moreover, the study further reveals that findings indicates WISE1810 could more likely to be associated with the Milky Way’s thick disk, despite its very low metallicity.

For the latest tech news and reviews, follow Gadgets 360 on X, Facebook, WhatsApp, Threads and Google News. For the latest videos on gadgets and tech, subscribe to our YouTube channel. If you want to know everything about top influencers, follow our in-house Who’sThat360 on Instagram and YouTube.


Red Magic 10 Air Launch Set for April 16; Colour Options Revealed



Vivo X200 Ultra Photography Kit Design, Key Features Revealed Ahead of April 21 Launch

Continue Reading

Science

Scientists Finally Discover How Long a Day Lasts on Uranus

Published

3 days ago

on

April 12, 2025

By

Scientists Finally Discover How Long a Day Lasts on Uranus

Scientists have finally found how about Uranus day length using the most recent analysis of a decade’s worth of Hubble Space Telescope data. As per the scientists, the Uranus holds 17 hours, 14 minutes, and 52 seconds to finish a complete rotation—that is, 28 seconds more than the estimation served by NASA’s Voyager 2 spacecraft. This estimation was made possible through the measurement of the magnetic fields and the radio waves coming from the auras of the planet. This understanding helps one derive surface mapping and alignment estimation in perplexing surroundings. Some of those maps may need to be reconsidered based on the most recent research.

Hubble Refines Uranus’ Spin and Orbit Time

According to reports, the Hubble Space Telescope study verified Uranus completed a revolution in 17 hours, 14 minutes, and 52 seconds. That is 28 seconds more than the NASA mission Voyager 2, from the 1980s.

The report further mentions that through examination of a ten-year record of aurora observations, a team headed by Laurent Lamy at the Paris Observatory in France revealed the magnetic poles of the planet. That long-term monitoring gave even more exact rotation periods—that is, nearly 84 Earth years for Uranus to orbit the sun.

Uranus’ Rotation Refined, Aiding Future Exploration

On Uranus, a day just lasts far longer. More precise rotational time observations of the gas giant should enable scientists to plan visits to investigate it. Unlike on Mars and Earth, savage windstorms make it far more difficult to identify the rotation times of the biggest solar system planets.

The first estimate of Uranus’s spin was shifted closer to the Voyager 2 probe, which made a close-range approach on January 24, 1986. The researchers during that time found out that the planet’s mangetic field was by 59 degrees from celestial north. Moreover, the researchers observed that its rotation axis was 98 degrees offset.

Uranus Spins Sideways with a 17-Hour Day, Scientists Confirm

The report further mentions that Uranus effectively revolves “lying down” compared to Earth; during this period, its magnetic poles find a giant circle as the planet rotates. These highest offsets mean With a safety margin of plus or minus 36 seconds, scientists at the time estimated that Uranus was completing a full revolution in every 17 hours, 14 minutes, and 24 seconds by measuring the magnetic field of the planet as well as radio emissions from aurora at its magnetic poles.

Continue Reading

Science

Farallon Slab Beneath Midwest Pulls Crust Downward, Causing Widespread Thinning

Published

3 days ago

on

April 12, 2025

By

Farallon Slab Beneath Midwest Pulls Crust Downward, Causing Widespread Thinning

An underground structure beneath central United States has been observed dragging surface materials deep into the Earth. This movement has been linked to an old piece of crust lodged far below the Midwest. Researchers have said this action is pulling rocks from across the continent towards a funnel-shaped region. It is believed this process is causing parts of the crust to thin as material is drawn downward. This phenomenon has been found to affect areas beyond the immediate region.

Underground slab tied to crust loss beneath Midwest

According to the study published in Nature Geoscience, the phenomenon has been tied to the remains of a long-subducted tectonic plate known as the Farallon slab. This slab, which sits around 660 kilometres below the surface, was identified as the driving force behind what scientists refer to as cratonic thinning. Cratons are known to be the stable core regions of continental crust and upper mantle that usually do not undergo change.

The seismic mapping project was led by Junlin Hua during his postdoctoral work at The University of Texas at Austin. He now serves as a professor at the University of Science and Technology of China. In a statement, Hua explained that a wide region is showing signs of thinning. He stated that the study has brought forward a new explanation behind this change.

New seismic method uncovers ‘dripping’ lithosphere

To observe the changes taking place beneath North America, researchers used a method known as full-waveform inversion. This seismic imaging approach allowed them to map the subsurface in high detail. According to Thorsten Becker, Geophysics Chair at UT Austin, this technique offered a better understanding of the link between deep mantle regions and the lithosphere above.

Computer simulations were used to confirm the effect. When the slab was included, the downward movement was visible. When removed, no such feature appeared.

For the latest tech news and reviews, follow Gadgets 360 on X, Facebook, WhatsApp, Threads and Google News. For the latest videos on gadgets and tech, subscribe to our YouTube channel. If you want to know everything about top influencers, follow our in-house Who’sThat360 on Instagram and YouTube.


CMF Phone 2 Pro India Launch Set for April 28; CMF Buds 2, Buds 2a, Buds 2 Plus to Tag Along



WazirX’s Restructuring Scheme Approved by Over 93 Percent Creditors, Refunds to Start Soon

Continue Reading

Trending