Mars
... Life on Mars? •The conditions on Mars are rather different from Earth •Mostly colder temperatures •No oxygen, low air pressure •No liquid water •No large form of life on Earth survives these conditions •But some bacteria on Earth live in similar conditions! What would life on Mars look like? •Bacte ...
... Life on Mars? •The conditions on Mars are rather different from Earth •Mostly colder temperatures •No oxygen, low air pressure •No liquid water •No large form of life on Earth survives these conditions •But some bacteria on Earth live in similar conditions! What would life on Mars look like? •Bacte ...
Kepler`s Law Applied to the Planets 10 868 870 9.54 29.5 Saturn 13
... Earth gets behind Mars Earth at departure Total Mission Time: ~ 2.6 yrs ...
... Earth gets behind Mars Earth at departure Total Mission Time: ~ 2.6 yrs ...
Venus and Mars - Mrs. Felker`s Science Site
... Young, uneven lava flows (shown: Lava flow near Flagstaff, AZ) show up as bright regions on radar maps. ...
... Young, uneven lava flows (shown: Lava flow near Flagstaff, AZ) show up as bright regions on radar maps. ...
document
... Scientific utility of the Copernican Heliocentric Model • Can deduce the true “sidereal” (as opposed to readily measured “synodic”) orbital periods of each of the planets [see textbook BOX 4-1 and Table 4-1] • Can deduce the distance that each planet is from the Sun, relative to the Earth’s distanc ...
... Scientific utility of the Copernican Heliocentric Model • Can deduce the true “sidereal” (as opposed to readily measured “synodic”) orbital periods of each of the planets [see textbook BOX 4-1 and Table 4-1] • Can deduce the distance that each planet is from the Sun, relative to the Earth’s distanc ...
Orbital distance 1.52 AU Orbital period 1.88 years Rotation period
... Spirit and Opportunity exploration [fig 11.27-30] further evidence of past water [mars_layered_rock_PIA05495.jpg, fig 11.31] Phoenix Mars Lander [fig 11.32,33 phoenix_scrape.jpg] ...
... Spirit and Opportunity exploration [fig 11.27-30] further evidence of past water [mars_layered_rock_PIA05495.jpg, fig 11.31] Phoenix Mars Lander [fig 11.32,33 phoenix_scrape.jpg] ...
Astronomy
... a) It has warm water b) It has an atmosphere like Earth c) Spectrographs have detected life’s chemical signature d) It has volcanoes 23. How could a rock from Mars end up on Earth? a) The rovers sent it back b) Astronauts brought it back c) A meteorite collision ejected material d) It was carried by ...
... a) It has warm water b) It has an atmosphere like Earth c) Spectrographs have detected life’s chemical signature d) It has volcanoes 23. How could a rock from Mars end up on Earth? a) The rovers sent it back b) Astronauts brought it back c) A meteorite collision ejected material d) It was carried by ...
Student 3
... the temperature hotter. Today the average temperature on mars is -63°C, liquid water only exists above 0°C. The most likely place for water to exist is underground or at the poles. The only obvious source of energy on Mars is the sun. If there were life on Mars it would likely take the form of plant ...
... the temperature hotter. Today the average temperature on mars is -63°C, liquid water only exists above 0°C. The most likely place for water to exist is underground or at the poles. The only obvious source of energy on Mars is the sun. If there were life on Mars it would likely take the form of plant ...
Mars: First Order Landforms
... Mars has one of the greatest eccentricities in the solar system at 0.0934 Earth is one of the more circular at 0.0167 ...
... Mars has one of the greatest eccentricities in the solar system at 0.0934 Earth is one of the more circular at 0.0167 ...
Modeling the Solar System - American Museum of Natural History
... From what students know about planets and space, along with what they observed in their models of the solar system, have them think about the challenges that humans would face in travelling to and living on another planet. Tell students that humans are most likely to return to the Moon and to visit ...
... From what students know about planets and space, along with what they observed in their models of the solar system, have them think about the challenges that humans would face in travelling to and living on another planet. Tell students that humans are most likely to return to the Moon and to visit ...
smallest exoplanet - Forsyth Astronomical Society
... shaped primarily by wind, rather than being cut into existing ice very recently. To view images and Mars Reconnaissance Orbiter info, see: http://www.nasa.gov/mro MARS PHOENIX LANDER NASA's Phoenix Mars Lander has ended operations after repeated attempts to contact the spacecraft were unsuccessful. ...
... shaped primarily by wind, rather than being cut into existing ice very recently. To view images and Mars Reconnaissance Orbiter info, see: http://www.nasa.gov/mro MARS PHOENIX LANDER NASA's Phoenix Mars Lander has ended operations after repeated attempts to contact the spacecraft were unsuccessful. ...
Venus and Mars
... Wrinkled mountain formations indicate compression and wrinkling, though there is no evidence of plate tectonics on Venus. ...
... Wrinkled mountain formations indicate compression and wrinkling, though there is no evidence of plate tectonics on Venus. ...
Here are some facts about my favorite objects in the Solar System, in
... Zealand to use a telescope there to watch Pluto go in front of a star. (Before we went to the telescope, we visited Sam's other grandparents, who live there.) Two weeks after we came back, on July 14, a NASA spacecraft called New Horizons went up close to Pluto after traveling there for 9 years. New ...
... Zealand to use a telescope there to watch Pluto go in front of a star. (Before we went to the telescope, we visited Sam's other grandparents, who live there.) Two weeks after we came back, on July 14, a NASA spacecraft called New Horizons went up close to Pluto after traveling there for 9 years. New ...
Homework #1 - Department of Physics and Astronomy
... northward at opposition. Make a diagram similar to Figure 1-1B, showing the retrograde path of this superior planet. ...
... northward at opposition. Make a diagram similar to Figure 1-1B, showing the retrograde path of this superior planet. ...
Terrestrial Planets
... Pluto in the Oort cloud, a spherical shell extending from 40,000 to 100,000 AU from the Sun • Some comets may also come from a disklike swarm of icy objects that lies beyond Neptune a region called the Kuiper Belt ...
... Pluto in the Oort cloud, a spherical shell extending from 40,000 to 100,000 AU from the Sun • Some comets may also come from a disklike swarm of icy objects that lies beyond Neptune a region called the Kuiper Belt ...
Mars
... • Phobos is the larger moon it orbits closer to the surface of Mars, Phobos orbits about twice a day around Mars, it orbits at an average distance of 9,377 km above Mars. • Demios orbits at an average distance of 23,460 km above Mars. Demios is much smaller than Phobos . It takes about 30.35 hours f ...
... • Phobos is the larger moon it orbits closer to the surface of Mars, Phobos orbits about twice a day around Mars, it orbits at an average distance of 9,377 km above Mars. • Demios orbits at an average distance of 23,460 km above Mars. Demios is much smaller than Phobos . It takes about 30.35 hours f ...
PTYS/ASTR 206 – Section 3 – Homework 4 – Assigned 3/12/09
... much energy each planet is producing per second. How much energy per second is being produced per kilogram for each planet (the masses of these planets are also in that table)? Are these numbers very different? Why do you suppose that is? ...
... much energy each planet is producing per second. How much energy per second is being produced per kilogram for each planet (the masses of these planets are also in that table)? Are these numbers very different? Why do you suppose that is? ...
IAF Pres. Draft
... Phase 1 – Introduction to Astrobiology Phase 2 – What is Needed for Life on Earth? Phase 3 – How to Look For, Protect & Study Life? Phase 4 – Which Planets/bodies in our Solar System are Best Suited to Contain Evidence of Life? Phase 5 – What We are Doing to Learn More About Possible Life Outside ou ...
... Phase 1 – Introduction to Astrobiology Phase 2 – What is Needed for Life on Earth? Phase 3 – How to Look For, Protect & Study Life? Phase 4 – Which Planets/bodies in our Solar System are Best Suited to Contain Evidence of Life? Phase 5 – What We are Doing to Learn More About Possible Life Outside ou ...
My Planet - Etiwanda E
... Unique / Interesting Facts • Mars travels around the Sun in an oval shaped pattern. • Mars is called The Red Planet because of its bright red color! • The first visit to Mars was in 1965 by the spacecraft Mariner 4. • One day on Mars is 24 hrs. 37 min. • One year on Mars is 687 Earth days! •http:// ...
... Unique / Interesting Facts • Mars travels around the Sun in an oval shaped pattern. • Mars is called The Red Planet because of its bright red color! • The first visit to Mars was in 1965 by the spacecraft Mariner 4. • One day on Mars is 24 hrs. 37 min. • One year on Mars is 687 Earth days! •http:// ...
Document
... The table below gives information about the planets of the Solar System. They are listed in alphabetical order. average distance from the Sun in million km ...
... The table below gives information about the planets of the Solar System. They are listed in alphabetical order. average distance from the Sun in million km ...
Solutions
... source of fuel is at the base. Assume that the buggies all have the same speed and fuel consumption throughout a journey, and that they all return safely to the base. What is the smallest number of buggies required to allow one buggy to complete a full circular trip around the Moon, passing over the ...
... source of fuel is at the base. Assume that the buggies all have the same speed and fuel consumption throughout a journey, and that they all return safely to the base. What is the smallest number of buggies required to allow one buggy to complete a full circular trip around the Moon, passing over the ...
Colonization of Mars
Mars is the focus of much speculation and scientific study about possible human colonization. Its surface conditions and the presence of water on Mars make it arguably the most hospitable of the planets in the Solar System, other than Earth. Mars requires less energy per unit mass (delta-v) to reach from Earth than any planet except Venus. However, at minimum energy use, a trip to Mars requires 6–7 months in space using current chemical spacecraft propulsion methods. Other challenges of human missions to Mars have been described.