Mars

Every two years, Earth and Mars change their orbits, significantly reducing the distance between the two planets.

These events are called solar eclipses because when Earth rotates, it shines at night.

It will be visible on July 27, and on July 31, the distance between the planets will be less than 93 million kilometers, which is less significant after 15 years.

This is not only a way to see and photograph Mars but also a way to understand Mars better.

Remember, every few years there is news that a rocket has landed on Mars.

Do not miss this year as well.

If all goes well, the launch of the spacecraft is scheduled for tomorrow morning with NASA’s InSight rover.

InSight’s mission is very different from other rovers that have reached Mars.

The goal of this mission is not to study and analyze materials on the surface of Mars or below it.

The aim of this year’s program is to gain a better understanding of Mars’s structure, especially its evolution.

The rocky planets of the Solar System—Mercury, Venus, Earth, and Mars—may have been created in the same way, but not necessarily.

It is known all over Mars (except on Earth).

By reading these signals, you can imagine where Mars is and how Earth has changed.

But what are the health signals?

This discovery is based on three main scientific tools: seismology, thermometry, and the precision of Mars’ albedo. At the moment, the Earth Inner Space Experiment (SEIS) uses onboard cameras and spacecraft probes to detect earthquakes (quakes on Mars).

It is very complicated, and we need to understand what can interfere with Mars’s orbit.

But the true reality is the effect of winds and storms caused by internal or external movements, currents, and flows.

After all, unlike Earth, seismography is very useful for determining Earth’s depth.

The so-called best thermometer is, in fact, a 1.5-meter stick that can be driven into the ground.

But the most surprising thing is that every half meter of the stick includes a generator that burns heat and controls pressure distribution in the soil.

The objective of the experiment is to study how heat is lost at different depths in various types of soil.

With this information, we can estimate how heat escapes from the planet’s core or how it must have escaped in the past.

The rocky planets are trapped in a warm interior and a cold exterior, forming a crust.

Over billions of years, internal heat has flowed through the structure and escaped into the atmosphere, warming the deeper layers.

In addition to heat released during its formation, the decomposition of Earth’s elements in the atmosphere produces a large amount of heat that follows the same paths through the inner layers before escaping into the atmosphere.

Earth Phenomenon on Mars

This is an earthly phenomenon and should reflect what we know about our planet and what has been studied on Mars.

A third important instrument is the RISE radio experiment, which consists of two antennas that, similar to Earth, rotate in a circular orbit around Mars, with the difference between the measured position and the estimated position being solely the rotation of “A.”

This slight instability shows the nature of the universe.

Whether Mars is thick or thin, it rotates in different directions; for example, we can imagine that Mars has more metal or more rock.

After all, NASA refers to the planet for temperature, pressure, and reflectance analysis.

The project is also testing new technologies.

InSight was a cube the size of two suitcases.

CubeSats are small satellites that use minimal technology and are currently used only in Earth’s orbit.

This is the first part of a larger section that could open doors for more information in the future.

Source of information: g1.globo.com

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