Connect with us

Published

on

NASA’s Hubble Space Telescope has given new insights into Jupiter’s Great Red Spot. Researchers have noticed that the speed of the winds in the massive planetary storm has increased over the last decade. This observation came after the analysis of Hubble’s regular “storm reports”. The average speed of the winds near the boundary has increased by 8 percent between the years 2009 and 2020. The current wind speed exceeds 400 miles per hour. This outer green circle is also called the high-speed ring. Interestingly, the winds at the vortex of the storm continue to move significantly slower.

The change in the peripheral wind speed recorded with the Hubble Space Telescope is, however, minuscule. The change amounts to less than 1.6 miles per hour per Earth year. Amy Simon, the NASA scientist who contributed to the research, said, “We’re talking about such a small change that if you didn’t have eleven years of Hubble data, we wouldn’t know it happened”.

The counter-clockwise and vortex spin of the massive storm is bigger than Earth. Astronomers have brooded over the Great Red Spot for almost 150 years, since the 1870s. The storm’s centre spurts out high clouds from Jupiter’s interior. These, then, run cascading down the sides over the outer layers of clouds. Its current diameter is 10,000 miles, which is almost three times bigger than the Earth’s diameter.

Michael Wong of the University of California, Berkeley, led the analysis and praised the Hubble Space Telescope for the data that led to the observation. “This is something only Hubble can do. Hubble’s longevity and ongoing observations make this revelation possible,” he said.

Scientists don’t have a storm chaser plane at Jupiter. That’s why they cannot continuously measure the winds on the planet. “Hubble is the only telescope that has the kind of temporal coverage and spatial resolution that can capture Jupiter’s winds in this detail,” said Simon. She added, “With Hubble, we have the precision we need to spot a trend”.

Wong analysed Hubble’s data by using software that tracked thousands of wind vectors whenever Hubble observed Jupiter. “I also ran a battery of statistical tests to confirm if it was justified to call this an increase in wind speed. It is,” he added.

In 2017, researchers also found an abrupt change in the storm’s wind speed when there was a major storm near the spot. Other recent observations about the Great Red Spot include the change in its size. Over a century’s observation shows that it has become more circular than oval.


This week on Orbital, the Gadgets 360 podcast, we discuss the Surface Pro 8, Go 3, Duo 2, and Laptop Studio — as Microsoft sets a vision for Windows 11 hardware. Orbital is available on Spotify, Gaana, JioSaavn, Google Podcasts, Apple Podcasts, Amazon Music and wherever you get your podcasts.

Continue Reading

Science

NASA’s X-59 Moves Closer to First Flight with Advanced Taxi Tests and Augmented Vision

Published

on

By

NASA’s X-59 Moves Closer to First Flight with Advanced Taxi Tests and Augmented Vision

X-59 of NASA has been designed from the ground to fly at a faster speed of sound without making thunderous sonic booms, which are usually associated with supersonic flight. This 99-foot aircraft, which features a logically elongated design, jettisons the front windscreen and is now heading towards the runway. Pilots can see what is at the front through an augmented reality (AR) enabled closed-circuit camera system, which is termed by NASA as the External Vision System (XVS). NASA took control of an experimental aircraft and performed taxi tests on it during this month.

X-59’s Futuristic Design: Eliminating Sonic Booms with External Vision System

According to As per NASA, the test pilot Nils Larson, during the test, drove the X-59 at the runway by keeping a low speed. This is done to ensure the working of the steering and braking systems of the jet. Lockheed Martina and NASA would perform the taxi tests at high speed, in which the X-59 will move faster to make it to the speed at which it will go for takeoff.

Taxi tests are held at the U.S. Air Force’s Plant 42 facility in Palmdale, California. The contractors and the Air Force utilise the plant for manufacturing and testing the aircraft. Lockheed Martin has developed this aircraft, whose Skunk Works is found in Plant 42.

Taxi Tests at Plant 42: NASA and Lockheed Martin Prepare X-59 for First Flight

Some advanced aircraft of the U.S. military were developed to a certain extent at Plant 42, together with the B-2 Spirit, the F-22 Raptor, and the uncrewed RQ-170 Sentinel spy drone.

SOFIA airborne observatory aircraft, which is a flying telescope called Plant 42, home recently retired. The space shuttle of the agency is the world’s first reusable spacecraft; these were assembled and tested at the facility.

Such taxi tests have started over the last months. NASA worked in collaboration with the Japan Aerospace Exploration Agency for testing a scale model of the X-59 in the supersonic wind tunnel to measure the noise created under the aircraft.

Continue Reading

Science

Unusual Plasma Waves Above Jupiter’s North Pole Can Possibly Be Explained

Published

on

By

Unusual Plasma Waves Above Jupiter’s North Pole Can Possibly Be Explained

In recent observations, NASA’s Juno spacecraft has significantly detected the presence of a variety of plasma waves. The emergence of these waves on Jupiter’s powerful magnetic field is projected to be surprising, as their existence was never marked in the planetary magnetospheres. However, scientists might have come out with an explanation. Furthermore, the current studies have been questioned by scientists surfacing the activity at the North Pole. The article below will exemplify the findings and shed light on the plasmas. 

Uncovering Mystery at Jupiter’s North Pole 

According to a paper published in the Physical Review Letters, the scientists have uncovered the explanation behind the presence of these strange waves. They mainly suspect that the formation of these waves lies behind their evolution as a plasma, which later transforms into something different. 

Inside Jupiter’s Plasmas and Their Variants 

Plasmas are best referred to as the waves that pass through the amalgamation of the charged particles in the planet’s magnetosphere.These plasma waves come across in two forms: One, Langmuir waves, which are high-pitched lights crafted with electrons, while the other, Alfven waves, are slower, formed by ions (heavy particles). 

About Juno’s Findings

As unveiled by the Juno, the findings turned out to be questionable after the scientists noted that in Jupiter’s far northern region, the plasma waves were relatively slower. The magnetic field is about 40 times stronger than the Earth’s, but scientists were shocked to witness the results as the waves were slower. To analyse this further, a team from the University of Minnesota, led by Robert Lysak, identified the possibility of Alfven waves transforming into Langmuir waves. Post studying the data extracted from the Juno, the researchers then began to compare the relationship between the plasma wave frequency and number. 

According to Lysak’s research team, near Jupiter’s north pole, there might be a potential pathway of Alfven waves, which are massive in numbers, transforming into Langmuir waves. Scientists are also predicting that the reason behind evolution might be strong electrons that are shooting upwards at a very high energy. This discovery was made in the year 2016. Considering the current findings, the researchers indicate that Jupiter’s magnetosphere may comprise a new type of plasma wave mode that occurs during high magnetic field strength. 

Continue Reading

Science

Russia Expands Space Weather Network, Launches Iran’s Nahid-2 in Joint Mission

Published

on

By

Russia Expands Space Weather Network, Launches Iran’s Nahid-2 in Joint Mission

Russia sent two new Ionosfera-M satellites into orbit on a Soyuz-2 on July 25, 2025. Rocket 1b from the Vostochny Cosmodrome in Siberia. The mission also placed Iran’s Nahid-2 communications satellite in orbit. These satellites will complement a four-satellite constellation aimed at keeping track of Earth’s upper atmosphere and space weather conditions, particularly the solar wind that can knock satellites and communications systems offline. The flight indicates Russia’s scientific ambitions and collaboration with Iran’s space program, showing Russia’s function in launching Tehran’s orbital assets. Both countries gain from the collaborative mission.

Russian Space Weather Satellites

According to official sources, Russia’s new Ionosfera-M probes, 3 and 4, follow two identical satellites launched in November 2024. Together the four craft form a mini-constellation orbiting about 820 kilometers above Earth. The network is explicitly designed to study space weather in the ionosphere, the charged upper atmosphere.

It will track solar wind and related phenomena that can disturb communications and navigation systems. The latest pair is being inserted into an orbital plane perpendicular to the first two, greatly expanding three-dimensional coverage of near-Earth space. They also carry a new Ozonometr-TM instrument to measure upper-atmosphere ozone for the first time in this mission.

Iranian Payload and International Implications

An Iranian communications satellite, Nahid-2, was also aboard the Soyuz mission.Nahid-2 is intended to bolster Iran’s civilian communications in space, an important capability given Iran’s limited homegrown launch capabilities. Russia’s role in the delivery of the payload reflects cooperation between the countries in space technology.

With the help of Russia, Iran can continue its satellite building efforts, even though these are restricted by the international community from also involving rocket export limitations. That Moscow has such a product even while Iran is under sanctions underscores the depth of their two-nation space partnership. This mission represents Russia’s support for ally’s space aspirations and the broader geopolitical implications of such collaborative efforts.

Continue Reading

Trending