NASA Returns To Mercury in 2011 with MESSENGER

Сентябрь 3, 2022

Главная
Астрономия
NASA Returns To Mercury in 2011 with MESSENGER

Содержание

2. This is the first mission to Mercury since Mariner 10 in 1975 It will fully map
3. Key questions for MESSENGER to answer: Why is Mercury so dense and iron-rich? What is the
4. What do we already know about Mercury? Mercury’s density is the highest of any planet It’s
5. MESSENGER was launched on August 3, 2004 from Cape Canaveral Air Force Station, Florida The probe
6. MESSENGER used gravity assists from Earth, Venus, and Mercury to lower its speed Each gravity assist
7. On March 18, 2011, the MESSENGER spacecraft will enter into orbit around Mercury, becoming the first
8. The spacecraft will have an extremely elliptical orbit of Mercury at an altitude of 200 km
9. Solar Panel Sunshade Main Thruster Instruments Fuel Storage Magnetometer Instrument
10. MESSENGER’S instruments: MDIS (Mercury Dual Imaging System)—map landforms, gather topographic information GRNS (Gamma-Ray and Neutron Spectrometer)—map
11. Systems MESSENGER’S instruments: MLA (Mercury Laser Altimeter—measure the amount of time for light to go to
12. On June 21, 2006 MESSENGER performed its final flip maneuver to keep its sunshade toward the
13. On June 5, 2007 Messenger made its closest approach to Venus and sent back data on
14. Scientists pored over the 614 images of Venus sent back from Messenger that helped them calibrate
15. On October 6, 2008, the MESSENGER spacecraft passed a mere 200 kilometers (124 miles) above Mercury's
16. First image of the previously unseen side of Mercury.
17. As MESSENGER sped by Mercury on January 14, 2008, the Narrow Angle Camera (NAC) of the
18. Credit: NASA/Johns Hopkins University Applied Physics Laboratory/Carnegie Institution of Washington Machaut is the name of a
20. Скачать презентацию

Слайд 2

This is the first mission to Mercury since Mariner 10 in

1975
It will fully map the entire surface of Mercury
It is carrying instruments to study mysteries of Mercury’s geology, thin atmosphere, tiny polar caps, and magnetic field

Слайд 3

Key questions for MESSENGER
to answer:
Why is Mercury so dense and iron-rich?

What is the geologic history of Mercury?
What is the structure of Mercury's core?
What is the nature of Mercury's magnetic field?
What are the unusual materials at Mercury's poles?

Слайд 4

What do we already know about
Mercury?
Mercury’s density is the highest of

any planet
It’s exotic atmosphere is the thinnest among all the terrestrial planets
It is the only terrestrial planet, besides Earth, to possess a magnetic field
Temperatures on Mercury vary from the highest in the solar system at its equator to among the coldest in its permanently shadowed poles

Слайд 5

MESSENGER was launched on August 3, 2004 from Cape Canaveral Air

Force Station, Florida
The probe used flybys of Earth, Venus, and is using Mercury itself to get into Mercury’s orbit
The trip to Mercury is taking 7 years, but scientific research will be possible during that time.

Слайд 6

MESSENGER used gravity assists from Earth, Venus, and Mercury to lower

its speed
Each gravity assist changed the shape, and tilt of MESSENGER’S orbit to get it ready for orbit insertion
The first of two gravity assist flybys of Venus occurred on October 24, 2006.
A second of two gravity assisted flybys of Venus occurred on June 5, 2007.

Слайд 7

On March 18, 2011, the MESSENGER spacecraft will enter into orbit

around Mercury, becoming the first spacecraft ever to orbit the Solar System's innermost planet.

Слайд 8

The spacecraft will have an extremely elliptical orbit of Mercury at

an altitude of 200 km (124 miles) at its lowest point and more than 15,193 km (9,420 miles) at its highest
MESSENGER’S 12-month orbit will cover 2 Mercury solar days (sunrise to sunrise) which is equal to 176 Earth days

Слайд 9

Solar Panel
Sunshade
Main Thruster
Instruments
Fuel Storage
Magnetometer
Instrument

Слайд 10

MESSENGER’S instruments:
MDIS (Mercury Dual Imaging System)—map landforms, gather topographic information
GRNS (Gamma-Ray

and Neutron Spectrometer)—map surface elements on Mercury to determine if there is ice at the poles
XRS (X-Ray Spectrometer)—detect emitted x-rays to measure various elements in the crust
MAG (Magnetometer)—map Mercury’s magnetic field

Слайд 11

Systems
MESSENGER’S instruments:
MLA (Mercury Laser Altimeter—measure the amount of time for light

to go to the surface and back to map topography
MASCS (Mercury Atmospheric and Surface Composition Spectrometer)—measure atmospheric gases and minerals on the surface
EPPS (Energetic Particle and Plasma Spectrometer)—analyze Mercury’s atmosphere
RS (Radio Science)—study Mercury’s mass and thickness of it’s crust

Слайд 12

On June 21, 2006 MESSENGER performed its final flip maneuver to

keep its sunshade toward the Sun
The sun is up to 11 times brighter on Mercury than we see on Earth and surface temperatures can reach 450°C (840°F)
The sunshade of heat-resistant ceramic cloth will keep MESSENGER operating at room temperature

Слайд 13

On June 5, 2007 Messenger made its closest approach to Venus

and sent back data on the planet
Venus Express is presently orbiting Venus, and the two spacecrafts sent back complimentary data on cloud structure, atmospheric conditions, magnetic fields, and atmospheric oxygen airglow

Messenger’s MDIS camera took this picture
on June 5 of Venus enshrouded in clouds

Слайд 14

Scientists pored over the 614 images of Venus sent back from

Messenger that helped them calibrate the MDIS camera in preparation for its first flyby of Mercury on January 14, 2008

Слайд 15

On October 6, 2008, the MESSENGER spacecraft passed a mere 200

kilometers (124 miles) above Mercury's surface for the mission's second flyby of its target planet.

Слайд 16

First image of the previously unseen side of Mercury.

Слайд 17

As MESSENGER sped by Mercury on January 14, 2008, the Narrow

Angle Camera (NAC) of the Mercury Dual Imaging System (MDIS) captured this image before its closest approach with the planet. The scene is near Mercury's terminator (the line between the sunlit day side and dark night side of the planet), where shadows are long and height differences accentuated, revealing rising crater walls that tower over the floors below.

Слайд 18