Planet Mars

Mars and Jupiter are two of the brightest objects in the night sky due to their size, proximity to Earth, and reflection of sunlight. Their orbits around the Sun also bring them close enough to Earth at certain times to be visible. Stargazers can easily spot them with the naked eye when they are above the horizon and conditions are clear.

Mars is to cold to have water. Plus its atmosphere is to thin.

Yes, but Mars does seem to have water ice at its poles. Also there is probably water under the surface, again in the form of ice.

Some challenges people face before traveling to Mars include prolonged space radiation exposure, muscle atrophy and bone density loss due to reduced gravity, psychological effects of isolation in a confined space for extended periods, and the need for advanced life support systems to sustain human life in the harsh Martian environment.

The first Land Rover sent to Mars was the Mars rover named "Sojourner," which was part of the Mars Pathfinder mission launched by NASA in 1996. It landed on Mars on July 4, 1997, and was the first rover to successfully operate on the Martian surface.

Launch dates:Mars 2(Prop-M) - 19th of May 1971

Mars 3(Prop-M) - 28th of May 1971

Sojourner - 4th of December 1996

PLUTO - 2nd of june 2003

Spirit - 10th of june 2003

Opportunity - 7th of July 2003

Curiosity - 26th of November 2011

No: it lacks a breathable atmosphere; it has no form of water on its surface (barring a small amount of polar ice); the temperature ranges across hundreds of degrees Celsius from night to day, and the extremes are well without human ability to stand unless they have some serious protective equipment.

It doesn't. It radios its data back to Earth. there is no need for the actual rover to come back. Nothing should be brought back from Mars unless it is proven lifeless, as Martian life may be dangerous to Earth life, like us!

The sand on Mars is primarily made up of basaltic rocks, which are the result of volcanic activity on the planet. Over time, these rocks eroded and crumbled into fine particles, creating the sandy surface that we see today. The wind then played a crucial role in shaping and moving these sand particles across the Martian landscape.

mars has different features the northern hemisphere is mostly plains with few craters the southern hemisphere has many craters and highlands

the surface of mercury look almost like our moon there are many caused by collision with meteoroids and comets there are smooth surface

earth is called the blue planet also has another feature that supports life -water it covers about 70 percent of the surface

venus the surface is highly eroded

Mars' weak gravity affects the planet in several ways. It means that objects weigh less on Mars compared to Earth, making it difficult to retain a thick atmosphere. This thin atmosphere also leads to weaker atmospheric pressure and lower temperatures on the planet. Additionally, the weaker gravity contributes to challenges for human exploration and potential colonization efforts.

Mars orbits the Sun at an average speed of about 24 kilometers per second (54,000 miles per hour). This orbital speed allows Mars to complete one orbit around the Sun in about 687 Earth days.

The average temperature on Mars is about 210 Kelvin (-63 degrees Celsius or -81 degrees Fahrenheit). However, temperatures can vary greatly depending on the location and time of day on the planet.

there are rings around Mars in fact there is a ring around every planet we can only see the one Saturn has and Uranus.

this answer might be wrong so don't use it because I only think it is this! but any bye!

Phobos is the smaller of the two moons of Mars, with a mean radius of about 11 kilometers. It is closer to Mars than its counterpart Deimos and orbits the planet in just 7 hours and 39 minutes.

Curiosity can hurt you if it leads you to dangerous or risky situations without proper preparation or knowledge. It can also be harmful if it distracts you from important responsibilities or causes you to invade someone else's privacy without their consent. Additionally, excessive curiosity can sometimes lead to unnecessary stress, anxiety, or obsession.

To convert your weight on Earth into your weight on Mars, you have to multiply your weight by 0.38.

So let's do the calculation for 94 pounds. 94 X 0.38 equals approx. 36. So you will weigh 36 lbs on Mars if you're 94 lbs on Earth.

yes it can,it can because there was once water and properties that we humans need today so by scientific research mars can support life
There is not one bit of oxygen on Mars, so humans do not have what they need to live most importantly which is oxygen.
We know that Mars cannot support Earth-like forms of life because there is very little atmosphere, very little water, and it is too cold. However, we cannot yet rule out the existence of other forms of life that perhaps once did, or perhaps still do, exist on the Red Planet.
to dry, no oxygen.
There is no oxygen, water or food.
no

Phobos and Deimos (Mar's moons) are not perfectly spherical. They are actually just captured asteroids. However, most moons and plants are round due to the following: Their is no gravity in space. So when the universe was formed, there were all these particles just floating around. All matter in space has their own gravitational field (a very small gravitational pull). When all that space dust was flying around, some of the particles got close enough to one another to stick (do to their individual gravitational pull). As more and more particles started sticking together, the gravitational pull gets stronger. As these masses were "growing" they "grew" evenly in all directions forming spherical entities.

Uranus's gravity is 90% that of Earth's, so if you weigh 100 lbs it's pretty simple, you would weigh 90 lbs on Uranus. You wouldn't last long there, though.

There Would Be Bad Air For Everyone.

If They Take Off Their Space Helmets,They Can't Breath.

There Would Be A Volcano On Mars.

You Would Be Bad To A Space Car.

Be Nice To Everything On Mars.

Analysis of materials from the Moon and Mars involves studying their composition, structure, and properties to understand their geological history and potential for supporting life. Scientists use techniques like spectroscopy and sample return missions to examine rocks, minerals, and gases from these bodies, providing insights into their past environment and evolution. This research can help in unraveling the mysteries of the solar system and inform future space exploration missions.

Mars is the fourth planet from the Sun in the Solar System. The planet is named after Mars, the Roman god of war. It is also referred to as the "Red Planet" because of its reddish appearance, due to iron oxide prevalent on its surface. Mars is a terrestrial planet with a thin atmosphere, having surface features reminiscent both of the impact craters of the Moon and the volcanoes, valleys, deserts and polar ice caps of Earth.

Unlike the Earth, Mars is now a geologically inactive planet with no known tectonic activity. It is the site of Olympus Mons, the highest known mountain in the Solar System, and of Valles Marineris, the largest canyon. The smooth Borealis basin in the northern hemisphere may be a giant impact feature covering 40% of the planet. Mars' rotational period and seasonal cycles are likewise similar to those of Earth.

Until the first flyby of Mars by Mariner 4 in 1965, many speculated that there might be liquid water on the planet's surface. This was based on observed periodic variations in light and dark patches, particularly in the polar latitudes, which looked like seas and continents, while long, dark striations were interpreted by some as irrigation channels for liquid water. These straight line features were later explained as optical illusions. Still, of all the planets in the Solar System other than Earth, Mars is the most likely to harbor liquid water, and thus may contain life.Geological evidence gathered by unmanned missions suggests that Mars once had large-scale water coverage on its surface, while small geyser-like water flows may have occurred during the past decade. In 2005, radar data revealed the presence of large quantities of water ice at the poles and at mid-latitudes (November 2008). The Phoenix Mars Lander directly sampled water ice in shallow martian soil on July 31, 2008.

Mars has two moons, Phobos and Deimos, which are small and irregularly shaped. These may be captured asteroids, similar to 5261 Eureka, a Martian Trojan asteroid. Mars can be seen from Earth with the naked eye. Its apparent magnitude reaches −2.91, a brightness surpassed only by Venus, the Moon, and the Sun, although most of the time Jupiter will appear brighter to the naked eye than Mars. Mars has an average opposition distance of 78 million km but can come as close as 55.7 million km during a close approach, such as occurred in 2003.

Mars is currently host to three functional orbiting spacecraft: Mars Odyssey, Mars Express, and the Mars Reconnaissance Orbiter. On the surface are the two Mars Exploration Rovers (Spirit and Opportunity) and several inert landers and rovers, both successful and unsuccessful. The Phoenix lander completed its mission on the surface in 2008. Observations by NASA's now-defunct Mars Global Surveyor show evidence that parts of the southern polar ice cap have been receding

Yes, there are meteorites on Mars that have hit the planet's surface. These meteorites are pieces of rock or metal from space that have traveled through space before crashing onto Mars. They provide valuable information about Mars' geology and history.