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
Sol Location in the Milky Way Galaxy
Local Fluff of Local Bubble
Galactic Orion Arm Spur
26,000 LY from Galactic Center
The Sun is 8.3 Light Minutes Away from Earth
Sol
1 estrella
9,941 F Photosphere
Sol
0.387 AU
Tidally Locked
0.01 Axial Tilt
176 Days Day
88 Day Year
Mercurian
0.055 (EM)
3,032 Miles
5.43 Density
0.38 g
Tenuous
6.6 Flux
Moderate Flares
Sol
0.723 AU
Not Locked
177.3 Axial Tilt
243 Days Day
225 Days Year
Terran
0.815 (EM)
7,520 Miles
5.24 Density
0.91 g
Toxic
1.9 Flux
Sol
1.000 AU *
Not Locked
23.5 Axial Tilt
24 Hour Day
365 Day Year
Terran
1.000 (EM)
7,926 Miles
5.52 Density
1.00 g
Breathable
1.0 Flux
Warm
Sol
1.523 AU *
Not Locked
25.2 Axial Tilt
24.4 Hour Day
687 Day Year
Sub Terran
0.107 (EM)
4,220 Miles
3.93 Density
0.38 g
Toxic
0.43 Flux
Sol
5.203 AU
Not Locked
3.13 Axial Tilt
9.9 Hour Day
11.86 Years Year
Super Jovian
317.83 (EM)
88,846 Miles
1.33 Density
2.40 g
Toxic
Frozen
0.037 Flux
4.3-14 Mag
No Life
Sol
2.2 to 3.2 AU
Main Sequence
4.603 Billion Years Old
Population I Star
Heavy Element Rich
No Life
Life ?
0.004 Mag
Hot
No Life
0.0003 Mag
Extremely Hot
0.65 Mag
0.02 Mag
Freezing
4.5 Billion *
4.53 Billion *
4.543 Billion *
4.56 Billion *
4.567 Billion *
Formed 5th
Formed 6th
Formed 7th
Formed 8th
Formed 1st
Sol
9.538 AU
Not Locked
26.73 Axial Tilt
10.7 Hour Day
29.45 Years Year
Jovian
95.161 (EM)
74,898 Miles
0.687 Density
0.91 g
Toxic
Frozen
0.011 Flux
0.2-0.8 Mag
No Life
4.566 Billion *
Formed 2nd
Sol
19.819 AU
Not Locked
97.77 Axial Tilt
17.4 Hour Day
84 Years Year
Neptunian
15.536 (EM)
31,518 Miles
1.27 Density
0.90 g
Toxic
Frozen
0.0027 Flux
1.1 Mag
No Life
Sol
30.058 AU
Not Locked
28.32 Axial Tilt
16 Hour Day
165 Years Year
Neptunian
17.148 (EM)
30,598 Miles
1.638 Density
1.14 g
Toxic
Frozen
0.0011 Flux
1.0 Mag
No Life
4.563 Billion *
4.562 Billion *
Formed 3rd
Formed 4th
1 AU (Astronomical Unit) = 92,955,807 Miles
Stellar Flux = How much sunlight energy per unit area a planet receives from the Sun
* = Age of the Planet in Years
* = Planet orbits within the Habitable Zone of its star, where liquid water is possible but not guaranteed
Sol Planets Probability to Host Life
Sol I (Mercury): Mercury's environment is not conducive to life as we know it. The temperatures and solar radiation that characterize Mercury are most likely too extreme for organisms to adapt to or thrive.
Sol II (Venus): The possibility of life on Venus is highly debated. While the surface conditions of Venus are extremely harsh (extremely hot, dry, and with a thick, acidic atmosphere), some scientists speculate that the clouds of Venus might offer a more habitable environment, potentially harboring microbial life. This is supported by the detection of phosphine, a gas that could be a biosignature, though this finding is still under investigation, and might be attributable to geological processes.
Sol III (Earth): The planet Earth, or Sol Prime, is the only known planet to host a complex variety of life, including micro-organisms, plants, animal, and Humans. Earth has an ideal environment with oceans of liquid water and continents to support life.
Sol IV (Mars): Ancient Mars is thought to have had a warmer, wetter climate with liquid water on its surface, potentially making it habitable for micro-organisms. Evidence suggests the planet had oceans of water and an atmosphere that could have supported life. However, Mars has since become a cold, dry, and radiation-exposed environment, raising questions about the survival of any life that may have existed.
The harsh surface conditions on Mars make it unlikely to find life on its surface. Subsurface environments, such as deep underground or near the poles (where ice melts), are potential areas where liquid water could exist and provide a refuge for life. Extremophiles, which are organisms that can survive in extreme conditions, offer clues about the types of life that might be able to exist on Mars. Methane has been detected on Mars, but its origin (biological or geological) is not yet confirmed.
Sol V (Jupiter): Jupiter's atmosphere contains chemicals necessary for life, and certain altitudes within its cloud structure offer suitable temperatures and potential energy sources from lightning. Water activity within Jupiter's clouds could be sufficient to support some forms of life. However, there are at least three major challenges when it comes to possible life in the clouds of Jupiter.
The first challenge is instability within Jupiter's clouds. Jupiter's strong winds could easily transport organisms to unfavorable depths where they would be scorched by heat or exposed to radiation. The second challenge is radiation from space. The upper atmosphere of Jupiter is exposed to intense radiation from space, which could damage or kill any life forms present in its clouds. The third challenge is nutrients. While the possibility of life based on water activity might be present, it doesn't address the availability of other essential nutrients that life might need to thrive.
Sol VI (Saturn): The chances of life on Saturn itself are extremely slim due to its harsh conditions, but some of its moons, particularly Titan and Enceladus, offer more promising possibilities. Saturn's extreme temperatures, pressures, and composition make it inhospitable for life as we know it. Saturn's atmosphere is extremely cold and turbulent, with winds reaching 1,100 mph. It's composed primarily of hydrogen and helium, with trace amounts of methane and other gases. Saturn lacks a solid surface and would crush anything that tried to descend into the depths of its clouds.
Saturn is a Gas Dwarf, meaning it doesn't have a solid surface like Earth, making it impossible for life as we know it to take hold on the planet itself. However, while life on Saturn itself is highly unlikely, some scientists speculate that extremophile organisms, which thrive in extreme environments, could potentially exist in the upper atmosphere of Saturn where conditions might be marginally less hostile.
Sol VII (Uranus): The environment of Uranus is not conducive to life as we know it on Earth. The temperatures, pressures, and materials that characterize Uranus are most likely too extreme and volatile for organisms to adapt to or thrive.
Sol VIII (Neptune): The possibility of life in Neptune's clouds is extremely low for several reasons including extreme temperatures, intense weather and wind, high pressure, volatile environment, and limited energy sources. Conditions within deeper parts of Neptune's atmosphere would likely be too extreme for life to adapt. Neptune is also extremely far from the Sun, receiving little solar energy. Internal heat drives Neptune's weather, but its suitability as a primary energy source for life is questionable.
Top 5 Most Asked Questions About the Solar System (Answered Simply)
What is the order of the planets in the Solar System?
The order of the planets in the Solar System, starting from the Sun, is: Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus, and Neptune. This sequence is based on each planet’s distance from the Sun, with Mercury being the closest and Neptune the farthest.
There are eight recognized planets in total. Pluto used to be considered the ninth planet, but it is now classified as a dwarf planet because it doesn’t meet all the criteria required to be a full planet.
How many planets are in the Solar System and why isn't Pluto one anymore?
There are eight planets in the Solar System: Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus, and Neptune. These are the officially recognized planets that orbit the Sun and meet the scientific criteria for planethood.
Pluto is no longer classified as a full planet because it doesn’t “clear its orbit,” meaning it shares its space with other objects in the Kuiper Belt. In 2006, the International Astronomical Union redefined what counts as a planet, and Pluto was reclassified as a dwarf planet based on those updated rules.
What is the largest planet in the Solar System?
The largest planet in the Solar System is Jupiter. It’s a gas giant made mostly of hydrogen and helium, and it’s so massive that it contains more than twice the mass of all the other planets combined. Jupiter’s diameter is about 11 times wider than Earth, making it the most dominant planet in the system.
Jupiter is also known for its powerful storms, including the famous Great Red Spot, a giant storm that has been raging for hundreds of years. Its strong gravity and many moons make it a key object of study in understanding how planetary systems form and evolve.
How did the Solar System form?
The Solar System formed about 4.6 billion years ago from a massive cloud of gas and dust in space. This process is explained by the nebular hypothesis, which describes how gravity caused the cloud to collapse and spin, forming a hot, rotating disk.
At the center of this disk, most of the material collected to form the Sun, while the remaining dust and gas gradually clumped together to form planets like Earth, Mars, and the other worlds in the system. Over time, these objects cooled and settled into the stable orbital system we see today.
Is there life anywhere else in the Solar System?
Right now, there is no confirmed evidence of life anywhere in the Solar System beyond Earth. Scientists have not found direct proof of living organisms, but several places are considered strong candidates for possible past or present microbial life.
The most promising locations include Mars, where ancient rivers once flowed, and icy moons like Europa (orbiting Jupiter) and Enceladus (orbiting Saturn), which likely have subsurface oceans beneath their ice crusts. These environments may have the water, energy, and chemistry needed for life as we understand it, making them key targets in the search for extraterrestrial biology.
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