Hubble Close to Mars in 2007

The Hubble Space Telescope Sees Mars's Close Approach in 2007
12.18.07
Credit: NASA, ESA, the Hubble Heritage Team (STScI/AURA), J. Bell (Cornell University), and M. Wolff (Space Science Institute, Boulder)
> Larger image NASA's Hubble Space Telescope took this close-up of the red planet Mars when it was just 55 million miles -- 88 million kilometers -- away. This color image was assembled from a series of exposures taken within 36 hours of the Mars closest approach with Hubble's Wide Field and Planetary Camera 2. Mars will be closest to Earth on December 18, at 11:45 p.m. Universal Time (6:45 p.m. EST).Mars and Earth have a "close encounter" about every 26 months. These periodic encounters are due to the differences in the two planets' orbits. Earth goes around the Sun twice as fast as Mars, lapping the Red Planet about every two years. Both planets have elliptical orbits, so their close encounters are not always at the same distance. In its close encounter with Earth in 2003, for example, Mars was about 20 million miles closer than it is in the 2007 closest approach, resulting in a much larger image of Mars as viewed from Earth in 2003.The two dominant dark swatches seen just south of the equator on this part of the planet are well observed regions that were originally labeled by early Mars observers. The large triangular shape to the right is Syrtis Major. The horizontal lane to the left is Sinus Meridani. One of NASA's Mars Exploration Rovers, named "Opportunity," landed at the western end of this region in January 2004. At the intersection of these two features is the prominent Huygens crater with a diameter of 270 miles (450 kilometers). South of Huygens is the Hellas impact basin, with a diameter of 1,100 miles (1,760 km) and a depth of nearly 5 miles (8 km). Hellas was formed billions of years ago when an asteroid collided into the Mars surface.The planet appears free of any dust storms during this closest approach, however, there are significant clouds visible in both the northern and southern polar cap regions. The resolution is 13 miles (21 kilometers) per pixel.Related link:> Images and animations from Hubblesite.orgFor more information, contact:Ray Villard / Keith NollSpace Telescope Science Institute, Baltimore, Md.villard@stsci.edu / noll@stsci.eduJames BellCornell University, Ithaca, N.Y.jimbo@marswatch.tn.cornell.edu

NASA Deep Impact Begins Hunt for Aliens World




NASA's Deep Impact Begins Hunt for Alien worlds 02.07.08 This is an artist concept of Epoxi, which uses the Deep Impact spacecraft. Image credit: NASA/JPL› Full image and caption NASA's Deep Impact spacecraft is aiming its largest telescope at five stars in a search for alien (exosolar) planets as it enters its extended mission, called Epoxi
NASA's Deep Impact Begins Hunt for Alien Worlds - 02.07.08
This is an artist concept of Epoxi, which uses the Deep Impact spacecraft. Image credit: NASA/JPL
› Full image and caption NASA's Deep Impact spacecraft is aiming its largest telescope at five stars in a search for alien (exosolar) planets as it enters its extended mission, called Epoxi. Deep Impact made history when the mission team directed an impactor from the spacecraft into comet Tempel 1 on July 4, 2005. NASA recently extended the mission, redirecting the spacecraft for a flyby of comet Hartley 2 on Oct. 11, 2010. As it cruises toward the comet, Deep Impact will observe five nearby stars with "transiting exosolar planets," so named because the planet transits, or passes in front of, its star. The Epoxi team, led by University of Maryland astronomer Michael A'Hearn, directed the spacecraft to begin these observations Jan. 22. The planets were discovered earlier and are giant planets with massive atmospheres, like Jupiter in our solar system. They orbit their stars much closer than Earth does the sun, so they are hot and belong to the class of exosolar planets nicknamed "Hot Jupiters." However, these giant planets may not be alone. If there are other worlds around these stars, they might also transit the star and be discovered by the spacecraft. Deep Impact can even find planets that don't transit, using a timing technique. Gravity from the unseen planets will pull on the transiting planets, altering their orbits and the timing of their transits. "We're on the hunt for planets down to the size of Earth, orbiting some of our closest neighboring stars," said Epoxi Deputy Principal Investigator Drake Deming of NASA's Goddard Space Flight Center in Greenbelt, Md. Epoxi is a combination of the names for the two extended mission components: the exosolar planet observations, called Extrasolar Planet Observations and Characterization (Epoch), and the flyby of comet Hartley 2, called the Deep Impact Extended Investigation (Dixi). Goddard leads the Epoch component. More than 200 exosolar planets have been discovered to date. Most of these are detected indirectly, by the gravitational pull they exert on their parent star. Directly observing exosolar planets by detecting the light reflected from them is very difficult, because a star's brilliance obscures light coming from any planets orbiting it. However, sometimes the orbit of an exosolar world is aligned so that it eclipses its star as seen from Earth. In these rare cases, called transits, light from that planet can be seen directly. "When the planet appears next to its star, your telescope captures their combined light. When the planet passes behind its star, your telescope only sees light from the star. By subtracting light from just the star from the combined light, you are left with light from the planet," said Deming, who is leading the search for exosolar worlds with Deep Impact. "We can analyze this light to discover what the atmospheres of these planets are like." Deep Impact will also look back to observe Earth in visible and infrared wavelengths, allowing comparisons with future discoveries of Earth-like planets around other stars. NASA's Jet Propulsion Laboratory, Pasadena, Calif., manages Epoxi for NASA's Science Mission Directorate, Washington. The University of Maryland is the Principal Investigator institution. NASA Goddard leads the mission's exosolar planet observations. The spacecraft was built for NASA by Ball Aerospace & Technologies Corp., Boulder, Colo. For information about Epoxi, visit http://www.nasa.gov/epoxi . More information about JPL is at www.jpl.nasa.gov . More information about NASA programs is at www.nasa.gov .
Media contacts: DC Agle 818-393-9011Jet Propulsion Laboratory, Pasadena, Calif. agle@jpl.nasa.gov Nancy Neal 301-286-0039Goddard Space Flight Center, Greenbelt, MDNancy.N.Jones@nasa.gov Lee Tune 301-405-4679University of Maryland, College Parkltune@umd.edu

Exploration of Mars - Current and past Mission of Mars




Mars Exploration
Mars Exploration - History and possible future crewed missions
Mars Exploration Program
Time on Mars - Map showing the current time and illumination on Mars
Center for Mars Exploration
Mars Today - Current orbital position and model surface conditions
Live from Earth and Mars: Meteorology and Images
Viking Image Atlas of Mars
On-line Mars Atlas
Hubble images of Mars
Life on Mars and Martian Meteorites
Life on Mars?
Images of Mars Meteorite showing putative microfossils
Meteorites from Mars
Mars Meteorite Compendium


Missions to Mars
Current and Past Missions

Phoenix - NASA Mars Scout Lander (2007)
Mars Reconnaissance Orbiter - NASA Orbiter (2005)
Mars Exploration Rovers - Two NASA Rovers to Mars (2003)
Spirit
Opportunity
Mars Express - ESA Mars Orbiter and Lander (2003)
2001 Mars Odyssey - NASA Orbiter Mission to Mars (2001)
Mars Polar Lander - NASA attempted lander to Mars (1999)
Deep Space 2 - NASA attempted penetrator mission to Mars (1999)
Mars Climate Orbiter - NASA attempted orbiter to Mars (1998)
Nozomi (Planet-B) - ISAS (Japan) orbiter to Mars (1998)
Mars Global Surveyor - NASA Mars orbiter (1996)
Mars Pathfinder - NASA lander and rover to Mars (1996)
Mars 96 - Russian attempted mission to Mars (1996)
Mars Observer - NASA attempted mission to Mars (1992)
Phobos - Soviet missions to Mars (1988)
Viking - NASA orbiters/landers to Mars (1975)
Mars 6 - Soviet Mars lander (1973)
Mars 5 - Soviet Mars orbiter (1973)
Mariner 9 - NASA Mars orbiter (1971)
Mars 3 - Soviet Mars orbiter and lander (1971)
Mars 2 - Soviet Mars orbiter and lander (1971)
Mariner 7 - NASA Mars flyby (1969)
Mariner 6 - NASA Mars flyby (1969)
Mariner 4 - NASA Mars flyby (1964)
Mars Chronology - Timeline of all Mars missions
Future Missions
Proposals For Future Missions Selected - NASA Press Release (8 Jan 2007)
Mars 2007 and Beyond - Proposed Future Missions to Mars (2007)
Hypothetical Scenario for Crewed Mission
NASA Official: Dr. Ed Grayzeck
Curator:
Dr. David R. Williams
Version 2.0.1
Last updated: 01 August 2008

Atmosphere of Mars - Other Sources of Information

Mars has a very thin atmosphere composed mostly of the tiny amount of remaining carbon dioxide (95.3%) plus nitrogen (2.7%), argon (1.6%) and traces of oxygen (0.15%) and water (0.03%). The average pressure on the surface of Mars is only about 7 millibars (less than 1% of Earth's), but it varies greatly with altitude from almost 9 millibars in the deepest basins to about 1 millibar at the top of Olympus Mons. But it is thick enough to support very strong winds and vast dust storms that on occasion engulf the entire planet for months. Mars' thin atmosphere produces a greenhouse effect but it is only enough to raise the surface temperature by 5 degrees (K); much less than what we see on Venus and Earth.
Other Sources of Information McKay et al. Science Article - Summary of the article that started it all Images of Mars - from the NSSDC Catalog of Spaceborne Imaging Images of Mars - from the NSSDC Photo Gallery NASA Press Release on the Discovery Mars Fact Sheet NSSDC Mars Home Page Life on Mars Press Briefing on 19 March 1997 - NASA Press Release (97-03-14) AAAS Symposium on Mars life and sample return mission - NASA Press Release (98-02-09)
Possible Source Craters for Mars Meteorite Found - Press Release - 12 August 1996 Summary Page on the Mars Meteorite - Including images of ALH84001 Mars Meteorite Compendium - Johnson Space Center News and scientific papers on the Mars Meteorite - Lunar and Planetary Institute Photos of the meteorite - The electron microscopy which led to the discovery SNC Meteorites - General information on meteorites from Mars American Association for the Advancement of Science - News Release CNN On-Line Information -
Special section on the discovery

Red Planet and Satellites




MARS PLANET

Mars is the fourth planet from the Sun and the seventh largest
Mars (Greek: Ares) is the god of War.
The planet probably got this name due to its red color
orbit: 227,940,000 km (1.52 AU) from Sun
diameter: 6,794 km
mass: 6.4219e23 kg
Volume (1010 km3) 16.318 108.321 0.151
Equatorial radius (km) 3396.2 6378.1 0.532
Polar radius (km) 3376.2 6356.8 0.531
Volumetric mean radius (km) 3389.5 6371.0 0.532
Core radius (km) 1700 3485 0.488
Ellipticity (Flattening) 0.00648 0.00335 1.93
Mean density (kg/m3) 3933 5515 0.713
Surface gravity (m/s2) 3.71 9.80 0.379
Surface acceleration (m/s2) 3.69 9.78 0.377
Escape velocity (km/s) 5.03 11.19 0.450
GM (x 106 km3/s2) 0.04283 0.3986 0.107
Bond albedo 0.250 0.306 0.817
Visual geometric albedo 0.150 0.367 0.409
Visual magnitude V(1,0) -1.52 -3.86 -
Solar irradiance (W/m2) 589.2 1367.6 0.431
Black-body temperature (K) 210.1 254.3 0.826
Topographic range (km) 30 20 1.500
Moment of inertia (I/MR2) 0.366 0.3308 1.106
J2 (x 10-6) 1960.45 1082.63 1.811
Number of natural satellites 2 1
Planetary ring system No No
The first spacecraft to visit Mars was Mariner 4 in 1965.
Several others followed including Mars 2, the first spacecraft to land on Mars and the two Viking landers in 1976. Ending a long 20 year hiatus, Mars Pathfinder landed successfully on Mars on 1997 July 4. In 2004 the Mars Expedition Rovers "Spirit" and "Opportunity" landed on Mars sending back geologic data and many pictures; they are still operating after more than three years on Mars. In 2008, Phoenix landed in the northern plains to search for water. Three Mars orbiters (Mars Reconnaissance Orbiter, Mars Odyssey, and Mars Express) are also currently in operation.
Mars' Satellites Mars has two tiny satellites which orbit very close to the martian surface: Distance Radius Mass
Satellite (000 km) (km) (kg) Discoverer Date
--------- -------- ------ ------- ---------- ----
Phobos 9 11 1.08e16 Hall 1877
Deimos 23 6 1.80e15 Hall 1877