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0 - 20 años luz

Esta base de datos de estrellas y planetas está en constante evolución y expansión a medida que hay nuevos datos astronómicos disponibles.

/ Estrellas y planetas / Estrellas y planetas 0 a 20 años luz

Mars Location in the Milky Way Galaxy

Local Fluff of Local Bubble

Galactic Orion Arm Spur

26,000 LY from Galactic Center

Mars is 12.72 Light Minutes Away from Earth

Barren Planet Class

Sol

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1 estrella

0.107 Earth Mass

Sol

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5,827 Miles

Tidally Locked

0.000000018 (EM)

Asteroidan

13.8 Miles

1.88 Density

0.06 g

No Atmosphere

Freezing

No Life

-80 F Average Temp (Freezing)

Toxic Atmosphere

4,220 Mile Diameter

3.93 Density

0.38 g

Sol

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14,580 Miles

Tidally Locked

0.00000002 (EM)

Asteroidan

7.8 Miles

1.47 Density

0.03 g

No Atmosphere

Freezing

No Life

Mars Tilt Relative to the Plane of Solar System

Mars Axial Tilt

25.2°

Sol

Mars Seasons

Spring
Summer
Fall
Winter

Sol

Mars Atmosphere Composition and Pressure

Carbon Dioxide

95%

Nitrogen

3%

Argon

2%

0.006 to 0.01 Bar Atmospheric Pressure
Venus has an Extremely Low Surface Atmospheric Pressure due to a Very Thin Atmosphere

Mars Weather

Clouds

High Altitude
Carbon Dioxide

Low Altitude
Water Ice
 

Wind

6 to 100
Miles per Hour

Rain


None

Lightning

Faint, Neon Glows
in Dust Devils and Dust Storms

Mars Surface and Internal Composition

Crust

Tholeiitic Basalt Rock Feldspar Rock Pyroxene Rock

Solid Crust

No Plate Tectonics

Mantle

Iron Olivine Rock
Soft
Upper Mantle

Peridotite Rock
Solid
Lower Mantle

Outer Core

73%
Liquid Iron Metal

8%
Liquid Nickel Metal

19% Sulfur

Inner Core

80%
Solid Iron Metal

10%
Solid Nickel Metal

10% Sulfur / Oxygen

Surface Liquid


None
 

Surface Ice

North Polar Cap
Water Ice

South Polar Cap
Water and Carbon Dioxide Ice Mix

Sub-Surface Liquid

Water in
Mid-Crust Layer Fractures

Sub-Surface Ice

Water Ice Contaminated by Toxic Perchlorates

Mars Magnetic Radiation Shield

0.02 Gauss Magnetic Field Strength
Caused by the Small Size of Mars and the Rapid Cooling the Core of Mars

Mars Similarity to Earth

45%

Sol

Mars Alien Life Chance

72%

Sol

Chemical Rocket Travel Time

9 Earth Months

Fission Rocket Travel Time

45 Earth Days

Fusion Rocket Travel Time

22.5 Earth Days

Laser Light Sail Travel Time

11.25 Earth Days

Top 10 Most Asked Questions About the Planet Mars (Answered Simply)

Can Humans live on Mars?

Humans could potentially live on Mars in the future, but not without advanced technology and carefully built habitats. Mars has a thin atmosphere made mostly of carbon dioxide, extremely cold temperatures, high radiation exposure, and no breathable air or liquid water on the surface. To survive, people would need sealed living environments, oxygen production systems, reliable food growing methods, radiation shielding, and ways to extract water from Martian ice or underground sources.

Despite these challenges, Mars remains the most realistic planet for future human settlement because it has water ice, a day length similar to Earth, and resources that could help support long term colonies. Space agencies like NASA and companies like SpaceX are actively developing technologies aimed at making human life on Mars possible, though permanent settlement is still likely decades away.

Is there life on Mars?

Scientists have not found definitive evidence of life on Mars, but Mars remains one of the most promising places in our solar System to search for signs of past or present microbial life. Billions of years ago, Mars had rivers, lakes, and a thicker atmosphere, creating conditions that may have been suitable for simple life. Today, researchers are studying Martian rocks, underground ice, and traces of organic molecules to better understand whether life ever existed there.

Robotic missions from NASA, including the Perseverance rover, are collecting samples and analyzing Mars’s surface for chemical signatures linked to ancient habitability. While no living organisms have been discovered, the search for life on Mars is still one of the most important goals in planetary science.

Why is Mars red?

Mars appears red because its surface is covered in iron-rich minerals that have rusted over billions of years. This rust, known as iron oxide, mixes with fine dust across the planet’s rocky landscape, giving Mars its distinctive reddish orange color when viewed from space or from Earth.

Powerful winds regularly lift this reddish dust into the thin Martian atmosphere, making the entire planet appear even more red. Because of this striking color, Mars has long been known as the Red Planet, one of its most recognizable features in our solar system.

How long does it take to get to Mars?

A trip from Earth to Mars usually takes about 6 to 9 months, depending on the positions of the two planets in their orbits and the speed of the spacecraft. Because Earth and Mars are constantly moving around the Sun, missions are typically launched during special windows, about every 26 months, when the planets are closest in a favorable alignment.

Travel time can vary based on mission design and propulsion technology. Robotic spacecraft sent by NASA have reached Mars in roughly seven months, while future human missions may aim for faster travel if more advanced propulsion systems are developed.

How big is Mars compared to Earth?

Mars is much smaller than Earth, with a diameter of about 4,220 miles or 6,790 kilometers, compared to Earth’s 7,918 miles or 12,742 kilometers. This means Mars is roughly half the size of Earth in diameter and has only about 15% of Earth’s volume, making it a significantly smaller world overall.

Because Mars is smaller, its gravity is also weaker, about 38% of Earth’s gravity, so a person who weighs 100 pounds on Earth would weigh only about 38 pounds on Mars. Even though Mars is smaller, it still has mountains, valleys, polar ice caps, and seasons, making it one of the most Earth-like planets in our solar system.

Does Mars have water?

Yes, Mars does have water, but most of it is not in liquid form on the surface today. Instead, large amounts of water are locked up as ice in the polar caps and also buried underground. Scientists have also found evidence that ancient Mars once had rivers, lakes, and even possibly oceans billions of years ago.

Occasionally, there are signs that small amounts of salty liquid water may briefly form under specific conditions, but it quickly freezes or evaporates due to the planet’s thin atmosphere. Missions from NASA continue to study Mars to understand where its water went and how much may still exist beneath the surface.

How many moons does Mars have?

Mars has two small moons, named Phobos and Deimos. These moons are much smaller than Earth’s Moon and are irregular in shape, likely captured asteroids rather than objects formed alongside Mars.

Phobos orbits very close to Mars and is slowly spiraling inward, meaning it may eventually break apart or crash into the planet in the distant future. Deimos orbits farther away and moves more slowly, appearing more stable. Both moons were discovered in 1877 and continue to be studied by missions from NASA to better understand their origin.

What is Mars made of?

Mars is primarily made of rock and metal, similar to Earth. Its core is believed to be made of iron, nickel, and sulfur, surrounded by a rocky mantle and crust composed mainly of iron rich basaltic rock. This iron content is what gives Mars its reddish color when the surface dust oxidizes.

The planet’s surface is covered in fine dust and rocky debris, along with minerals such as iron oxides, silicates, and clays. In some regions, scientists have also detected signs of past volcanic activity and ancient water-altered minerals, which suggest Mars once had a much more active and potentially wetter geological history.

How cold is Mars?

Mars is extremely cold compared to Earth. The average temperature on the planet is about -80° F or -60°C, but it can vary widely depending on location and time of day. Near the equator, temperatures can rise to around 70° F or 20° C during the day, but at night they can drop sharply to -195°F or -125°C.

These extreme temperature swings happen because Mars has a very thin atmosphere, which cannot hold heat well. As a result, heat escapes quickly into space, making the planet one of the coldest environments in the solar system.

Could Mars be terraformed?

In theory, Mars could be terraformed, but it would require technology far beyond what humanity currently has. The main idea behind terraforming is to warm the planet, thicken its atmosphere, and introduce conditions that could support liquid water and eventually more Earth-like environments. However, Mars has a very thin atmosphere, low gravity, and no global magnetic field, which makes long term atmospheric stability extremely difficult.

Some proposed methods include releasing greenhouse gases to warm the planet, melting polar ice to release carbon dioxide and water vapor, or building large orbital mirrors to increase sunlight. Even with these ideas, most scientists believe full terraforming would take hundreds or thousands of years, if it is possible at all, though organizations like NASA continue to study Mars to better understand its potential for future human settlement rather than full planetary transformation.

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