Brazilian Astronomer Records Asteroid Impact on Jupiter, One of the Rare Events Observable from Earth
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Brazilian Astronomer Records Asteroid Impact on Jupiter, One of the Rare Events Observable from Earth

A Brazilian citizen documented a rare phenomenon—the collision of an asteroid with Jupiter, the gas giant. Asteroids are remnants of the formation of the Solar System, which occurred about 4.6 billion years ago. Many of them continue to orbit the Sun, primarily in the so-called Asteroid Belt located between Mars and Jupiter.

However, these orbits are not entirely stable and can change under the influence of planetary gravity, especially the strong influence of the gas giant. Due to its colossal mass, Jupiter exerts a powerful gravitational pull on surrounding objects, functioning as an extensive cosmic shield. This scenario leads to the planet regularly being struck by space rocks, although the vast majority of these events remain unnoticed by telescopes.

In certain cases, larger stones enter Jupiter's atmosphere, causing a brief flash of light. This brilliance lasts only a few seconds but possesses enough energy to be registered by instruments on Earth, overcoming distances of hundreds of millions of kilometers.

Event Recording

One such event occurred on September 13, 2021, and was recorded by an amateur astronomer from Brazil who was observing Jupiter and noticed a rapid flare caused by the impact. This recording helped document another rare episode that can be observed directly.

The person responsible for this achievement is José Luís Pereira, a retired civil engineer living in São Caetano do Sul (SP). In an interview with the program Olhar Espacial, he spoke about his experience. He noted how great it is to contribute to the field of astronomy, especially planetary astronomy, by collecting data that can be used by professionals.

The observer's interest in astronomy arose in childhood, and the decision to focus on planets was influenced by the urban environment, as excessive lighting hinders the observation of fainter celestial bodies. Pereira explained that due to the high level of light pollution in a large city, it was very difficult to find nebulae and galaxies, so he focused on the planetary region.

To deepen his analyses, Pereira began using software created by the Frenchman Marc Delcroix, designed to search for impacts on Jupiter. This program automatically analyzes hours of continuous recordings sent by volunteers from around the world, identifying any suspicious changes in the planet's luminosity.

Observation Details

The historical recording took place during a night of bad weather. The amateur astronomer struggled with high cloud cover in the sky when he noticed a glowing point. He recalls: 'In the first video, while I was focusing the telescope, I saw a white spot on the planet, but I thought it was related to the settings.' Confirmation came the next morning when the program analyzed the night files and indicated a high probability of an impact. He used the program to separate the video into images, after which he saw a clear sequence from the beginning of the flash to its diminishing and disappearance, concluding: 'Yes, it really was an impact.'

Excited by the discovery, he contacted the program creator to verify the file. The analysis showed the scale of the event: the object had a diameter of 5 to 20 meters and was moving at a speed of 60 kilometers per second, creating an explosion approximately 5,000 kilometers in extent. Pereira explained: 'This flare was estimated to be 5,000 km in diameter. Therefore, the light it created was visible here on Earth.'

Significance of Data Contribution

Recording such events requires immense dedication and thousands of hours of continuous observation through cameras. The astronomer stated that before this impact, he had accumulated 6.5 days of continuous observations, emphasizing that community involvement allows for the collection of significant amounts of data unavailable to professional researchers alone.

Obtaining clear images requires overcoming the turbulence of the Earth's atmosphere, which distorts light and makes the planet appear shaky. Pereira compares this to the feeling of 'observing through water, inside a pool.' To cope with this instability and achieve magnification of more than a thousand times, the engineer improved the mechanics of his telescope and built a small private observatory to protect the equipment from the wind.

According to Pereira, assembling equipment of this level is a gradual process carried out in stages by replacing cameras, mirrors, and computerized mounts. After creating the structure, he expanded his horizons in recent years: he acquired a specialized solar telescope and now also dedicates time to recording solar flares and filaments. Pereira's discovery demonstrates the value of amateur collaboration in mapping small bodies of the Solar System. Continuous recordings help scientists calculate the frequency of such episodes, expanding the understanding of impact risks threatening other worlds and our own planet.

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NASA identifies new crater on the Moon, larger than the Colosseum, resulting from asteroid or comet impact
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NASA identifies new crater on the Moon, larger than the Colosseum, resulting from asteroid or comet impact

The Lunar Reconnaissance Orbiter (LRO), belonging to NASA, detected a recently formed crater on the Moon. This impact, caused by an asteroid or comet between April and May 2024, resulted in the creation of the largest known impact crater in recent times, with a diameter of 222 meters.

The identification was made after scientist Robert Wagner conducted a detailed comparison of lunar surface images. The collision event dispersed material over a distance greater than 100 kilometers and showed soil modifications, information that may be useful for planning future lunar constructions.

Characteristics of the new formation

This structure, named McGetchin, has a width of 222 meters and reaches a depth of 43 meters. Its dimensions are comparable to the Colosseum, and its depth would be sufficient to house three stacked school buses.

It is estimated that the celestial body responsible for the collision was equivalent in size to a three-to-six-story building. Researchers point out that an impact of this magnitude occurs on the Moon at intervals of approximately a century or even longer periods.

The collision scattered dust and rocks over more than 100 kilometers. Additionally, another study observed an area of about 7 kilometers around the crater that exhibits a nighttime temperature about 9°C lower.

This phenomenon is associated with regolith, the surface layer composed of dust and fragments on the Moon. The impact made this material looser and less dense, decreasing its ability to retain heat.

Scientific implications and additional discoveries

David Paige, from the University of California, Los Angeles, drew an analogy between the process and soil cultivation. He explained that they are now analyzing the impacts as a way to 'cultivate' the regolith, by turning over sediments and exposing materials normally found beneath it to the surface.

The discovery occurred during a routine check when Wagner was comparing maps generated from images from different years and noticed a clear area surrounded by a dark region. He reported immediately stopping his work to investigate the point in question.

Although computational software flagged differences in the images, it generated many false alarms due to variations in shadow and lighting. Subsequent images captured by the high-resolution camera were crucial for confirming the crater, measuring its dimensions, and analyzing the impact effects.

Since 2009, the LRO has cataloged at least a thousand new craters and approximately one hundred thousand other changes on the lunar surface, caused by both impacts and the debris released by them.

The collected data also suggests that the top two centimeters of lunar soil are disturbed every 80,000 years, a faster rate than previously estimated. This movement implies that the marks left by Apollo mission astronauts will not remain intact for this period.

Currently, scientists are working to calculate the risk of materials launched by future impacts hitting a future lunar base. This calculation will assist engineers in designing structures more resistant to the effects of these collisions.

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