7.6: Missions to Mercury and Venus.
- Page ID
- 30902
\( \newcommand{\vecs}[1]{\overset { \scriptstyle \rightharpoonup} {\mathbf{#1}} } \)
\( \newcommand{\vecd}[1]{\overset{-\!-\!\rightharpoonup}{\vphantom{a}\smash {#1}}} \)
\( \newcommand{\id}{\mathrm{id}}\) \( \newcommand{\Span}{\mathrm{span}}\)
( \newcommand{\kernel}{\mathrm{null}\,}\) \( \newcommand{\range}{\mathrm{range}\,}\)
\( \newcommand{\RealPart}{\mathrm{Re}}\) \( \newcommand{\ImaginaryPart}{\mathrm{Im}}\)
\( \newcommand{\Argument}{\mathrm{Arg}}\) \( \newcommand{\norm}[1]{\| #1 \|}\)
\( \newcommand{\inner}[2]{\langle #1, #2 \rangle}\)
\( \newcommand{\Span}{\mathrm{span}}\)
\( \newcommand{\id}{\mathrm{id}}\)
\( \newcommand{\Span}{\mathrm{span}}\)
\( \newcommand{\kernel}{\mathrm{null}\,}\)
\( \newcommand{\range}{\mathrm{range}\,}\)
\( \newcommand{\RealPart}{\mathrm{Re}}\)
\( \newcommand{\ImaginaryPart}{\mathrm{Im}}\)
\( \newcommand{\Argument}{\mathrm{Arg}}\)
\( \newcommand{\norm}[1]{\| #1 \|}\)
\( \newcommand{\inner}[2]{\langle #1, #2 \rangle}\)
\( \newcommand{\Span}{\mathrm{span}}\) \( \newcommand{\AA}{\unicode[.8,0]{x212B}}\)
\( \newcommand{\vectorA}[1]{\vec{#1}} % arrow\)
\( \newcommand{\vectorAt}[1]{\vec{\text{#1}}} % arrow\)
\( \newcommand{\vectorB}[1]{\overset { \scriptstyle \rightharpoonup} {\mathbf{#1}} } \)
\( \newcommand{\vectorC}[1]{\textbf{#1}} \)
\( \newcommand{\vectorD}[1]{\overrightarrow{#1}} \)
\( \newcommand{\vectorDt}[1]{\overrightarrow{\text{#1}}} \)
\( \newcommand{\vectE}[1]{\overset{-\!-\!\rightharpoonup}{\vphantom{a}\smash{\mathbf {#1}}}} \)
\( \newcommand{\vecs}[1]{\overset { \scriptstyle \rightharpoonup} {\mathbf{#1}} } \)
\( \newcommand{\vecd}[1]{\overset{-\!-\!\rightharpoonup}{\vphantom{a}\smash {#1}}} \)
\(\newcommand{\avec}{\mathbf a}\) \(\newcommand{\bvec}{\mathbf b}\) \(\newcommand{\cvec}{\mathbf c}\) \(\newcommand{\dvec}{\mathbf d}\) \(\newcommand{\dtil}{\widetilde{\mathbf d}}\) \(\newcommand{\evec}{\mathbf e}\) \(\newcommand{\fvec}{\mathbf f}\) \(\newcommand{\nvec}{\mathbf n}\) \(\newcommand{\pvec}{\mathbf p}\) \(\newcommand{\qvec}{\mathbf q}\) \(\newcommand{\svec}{\mathbf s}\) \(\newcommand{\tvec}{\mathbf t}\) \(\newcommand{\uvec}{\mathbf u}\) \(\newcommand{\vvec}{\mathbf v}\) \(\newcommand{\wvec}{\mathbf w}\) \(\newcommand{\xvec}{\mathbf x}\) \(\newcommand{\yvec}{\mathbf y}\) \(\newcommand{\zvec}{\mathbf z}\) \(\newcommand{\rvec}{\mathbf r}\) \(\newcommand{\mvec}{\mathbf m}\) \(\newcommand{\zerovec}{\mathbf 0}\) \(\newcommand{\onevec}{\mathbf 1}\) \(\newcommand{\real}{\mathbb R}\) \(\newcommand{\twovec}[2]{\left[\begin{array}{r}#1 \\ #2 \end{array}\right]}\) \(\newcommand{\ctwovec}[2]{\left[\begin{array}{c}#1 \\ #2 \end{array}\right]}\) \(\newcommand{\threevec}[3]{\left[\begin{array}{r}#1 \\ #2 \\ #3 \end{array}\right]}\) \(\newcommand{\cthreevec}[3]{\left[\begin{array}{c}#1 \\ #2 \\ #3 \end{array}\right]}\) \(\newcommand{\fourvec}[4]{\left[\begin{array}{r}#1 \\ #2 \\ #3 \\ #4 \end{array}\right]}\) \(\newcommand{\cfourvec}[4]{\left[\begin{array}{c}#1 \\ #2 \\ #3 \\ #4 \end{array}\right]}\) \(\newcommand{\fivevec}[5]{\left[\begin{array}{r}#1 \\ #2 \\ #3 \\ #4 \\ #5 \\ \end{array}\right]}\) \(\newcommand{\cfivevec}[5]{\left[\begin{array}{c}#1 \\ #2 \\ #3 \\ #4 \\ #5 \\ \end{array}\right]}\) \(\newcommand{\mattwo}[4]{\left[\begin{array}{rr}#1 \amp #2 \\ #3 \amp #4 \\ \end{array}\right]}\) \(\newcommand{\laspan}[1]{\text{Span}\{#1\}}\) \(\newcommand{\bcal}{\cal B}\) \(\newcommand{\ccal}{\cal C}\) \(\newcommand{\scal}{\cal S}\) \(\newcommand{\wcal}{\cal W}\) \(\newcommand{\ecal}{\cal E}\) \(\newcommand{\coords}[2]{\left\{#1\right\}_{#2}}\) \(\newcommand{\gray}[1]{\color{gray}{#1}}\) \(\newcommand{\lgray}[1]{\color{lightgray}{#1}}\) \(\newcommand{\rank}{\operatorname{rank}}\) \(\newcommand{\row}{\text{Row}}\) \(\newcommand{\col}{\text{Col}}\) \(\renewcommand{\row}{\text{Row}}\) \(\newcommand{\nul}{\text{Nul}}\) \(\newcommand{\var}{\text{Var}}\) \(\newcommand{\corr}{\text{corr}}\) \(\newcommand{\len}[1]{\left|#1\right|}\) \(\newcommand{\bbar}{\overline{\bvec}}\) \(\newcommand{\bhat}{\widehat{\bvec}}\) \(\newcommand{\bperp}{\bvec^\perp}\) \(\newcommand{\xhat}{\widehat{\xvec}}\) \(\newcommand{\vhat}{\widehat{\vvec}}\) \(\newcommand{\uhat}{\widehat{\uvec}}\) \(\newcommand{\what}{\widehat{\wvec}}\) \(\newcommand{\Sighat}{\widehat{\Sigma}}\) \(\newcommand{\lt}{<}\) \(\newcommand{\gt}{>}\) \(\newcommand{\amp}{&}\) \(\definecolor{fillinmathshade}{gray}{0.9}\)7.6.1 Missions to Mercury
Getting to Mercury is not easy. That close to the Sun, a probe must contend with the high temperatures and the gravity of the Sun, either of which could jeopardize a mission to the smallest of the planets.
To date, only two probes have visited Mercury. Launched on November 3, 1973, Mariner 10 made its first flyby of Mercury on March 24, 1974. Later, it made two more passes on September 21, 1974 and March 16, 1974. Because the same side of Mercury was illuminated by the Sun on each flyby, however, Mariner 10 only mapped about 45% of the planet’s surface. Mariner 10 also detected a magnetic field around Mercury.

https:/www.needpix.com/photo/269915/mercury-planet-solar-system-space-travel-landing-technology-target-vision-brown;
The MErcury Surface, Space ENvironment, GEochemistry, and Ranging (MESSENGER) was launched on August 4, 2004 and made several passes around Earth, Venus, and Mercury from 2005-2008. MESSENGER entered orbit of Mercury in 2011. It made the first detailed observations of Mercury and exceeded its initial plans. MESSANGER managed to map the entire surface of Mercury. Then in 2015, after two mission extensions, it ran out of propellant was allowed to crash into the planet.
As of this writing, a third probe is en route to Mercury. BepiColombo, Joint ESA-JAXA mission to Mercury was launched on October 20, 2018. After making several passes around Venus and Earth, it is due to arrive in 2025. The mission comprises two spacecraft: The Mercury Planetary Orbiter (MPO) and the Mercury Magnetospheric Orbiter (MMO). BepiColombo will orbit Mercury as it attempts to determine if its core is solid or liquid, whether planet has any active plate tectonics, and learn more about Mercury’s composition.
7.6.2 Missions to Venus
Venus has posed other challenges to observers on Earth. Because of its extensive cloud cover, the surface of Venus cannot be mapped using visible light. In the 1960s, NASA’s Goldstone and the Arecibo telescope began using radar to map the planet This enabled us to determine the planet’s rotational period, axis of rotation, and planetary radius for the first time. From the sixties until the mid-eighties, the Soviet Union sent numerous probes to study Venus, most of which failed. While the Soviets were determined to land a probe on Venus, NASA launched relatively few probes to Venus, all of which were either flyby or orbiter missions.
Spacecraft |
Launch Date |
Operator |
Mission Type |
Result |
Tyazhely Sputnik |
2/4/61 |
USSR |
Impactor |
Launch failure |
Venera 1 |
2/12/61 |
USSR |
Impactor |
Spacecraft failure |
Mariner 1 |
7/22/62 |
NASA |
Flyby |
Launch failure |
2MV-1 No.1 |
8/25/62 |
USSR |
Lander |
Launch failure |
Mariner 2 |
8/27/62 |
NASA |
Flyby |
Successful |
2MV-1 No.2 |
9/1/62 |
USSR |
Lander |
Launch failure |
2MV-2 No. 1 |
9/12/62 |
USSR |
Flyby |
Launch failure |
2MV-2 No. 1 |
2/19/64 |
USSR |
Flyby |
Launch failure |
Kosmos 27 |
3/27/64 |
USSR |
Flyby |
Launch failure |
Zond-1 |
4/2/64 |
USSR |
Flyby/lander |
Spacecraft failure |
Venera 2 |
11/12/65 |
USSR |
Flyby |
Spacecraft failure |
Venera 3 |
11/16/65 |
USSR |
Lander |
Spacecraft failure |
Kosmo 96 |
11/23/65 |
USSR |
Flyby |
Launch failure |
Venera 4 |
6/12/67 |
USSR |
Atmospheric |
Successful (First manmade enter the atmosphere of Venus) |
Mariner 5 |
6/14/67 |
MASA |
Flyby |
Successful |
Kosmos 167 |
6/17/67 |
USSR |
Lander |
Launch failure |
Venera 5 |
1/5/69 |
USSR |
Atmospheric |
Successful |
Venera 6 |
1/10/69 |
USSR |
Atmospheric |
Successful |
Venera 7 |
8/17/70 |
USSR |
Lander |
Partially successful (Landed on its side, making it the first soft landing on another planet. Only returned partial data) |
Kosmos 359 |
8/22/70 |
USSR |
Lander |
Launch failure |
Venera 8 |
3/27/72 |
USSR |
Lander |
Successful |
Kosmos 482 |
3/31/72 |
USSR |
Lander |
Launch failure |
Mariner 10 |
11/3/73 |
NASA |
Flyby |
Successful |
Venera 9 |
6/8/75 |
USSR |
Orbiter/lander |
Successful |
Venera 10 |
6/14/75 |
USSR |
Orbiter/lander |
Successful |
Venera 11 |
9/9/78 |
USSR |
Flyby/lander |
Partially successful (some instruments failed) |
Venera 12 |
9/14/78 |
USSR |
Flyby/lander |
Partially successful (Both cameras on lander failed) |
Pioneer Venus 1 |
5/20/78 |
NASA |
Orbiter |
Successful |
Pioneer Venus 2 |
8/8/78 |
NASA |
Atmospheric |
Successful |
Venera 13 |
10/30/81 |
USSR |
Flyby/lander |
Successful |
Venera 14 |
11/4/81 |
USSR |
Flyby/lander |
Successful |
Venera 15 |
6/2/83 |
USSR |
Orbiter |
Successful |
Venera 16 |
6/7/83 |
USSR |
Orbiter |
Successful |
Vega 1 |
12/15/84 |
USSR |
Flyby/atmospheric/lander |
Successful |
Vega 2 |
12/21/84 |
USSR |
Flyby/atmosphere/lander |
Successful (last Soviet mission to Venus) |
Magellan |
5/4/89 |
NASA |
Orbiter |
Successful (Used Radar to map the planet) |
Galileo |
10/18/89 |
NASA |
Gravity assist |
Successful (gravity assist en route to Jupiter) |
Cassini |
10/15/97 |
NASA/ESA |
Gravity assist |
Successful (gravity assist en route to Saturn) |
MESSENGER |
8/4/04 |
NASA |
Gravity assist |
Successful (gravity assist en route to Mercury) |
Venus Express |
11/9/05 |
ESA |
Orbiter |
Successful |
Akatsuki |
5/20/10 |
JAXA |
Orbiter |
Successful (still operation) |
IKAROS |
5/20/10 |
JAXA |
Flyby |
Successful (experimental solar sail deployed by Akatsuki) |
Shin’en |
5/20/10 |
JAXA |
Flyby |
Spacecraft failure (communication lost and past Venus |
BepiColombo |
10/20/18 |
ESA/JAXA |
Gravity assist |
Successful (made two flybys for gravity assist en route to Mercury) |

https:/search.creativecommons.org/photos/41a0c0e4-af0d-48cd-8575-1db90b7c68dc;
Cloud cities on Venus?
Several agencies around the world have future missions planned or proposed for Venus. Some scientists have suggested that Venus might be the place to establish a cloud city, like the one portrayed in Star War: The Empire Strikes Back. Because carbon dioxide is heavier than breathable air, you could fill a balloon with a nitrogen/oxygen mix and it will float at that level. At about 30 miles about the surface, the pressure is close to that on Earth and the temperatures are more bearable than the hellish conditions on the surface. A 1-km diameter spherical balloon could lift 700,000 tons (about two Empire State Buildings) while a balloon 2-km in diameter could life 6 million tons! Colonists could (theoretically) live inside these balloon cities and use robots to mine the surface.
NASA has a proposal called HAVOC (High Altitude Venus Orbital Concept). This would involve sending astronauts to Venus with a dirigible that they could fill with ordinary air. They could then pilot this airship 30 miles above the surface where the pressure is close to that of the Earth.