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Pioneer Venus Multiprobe

Pioneer Venus Multiprobe is a science topic covered in the lgStudy science library. This page brings together a partial reference excerpt, illustrations, worked examples, real-world applications and a short study plan, so you can understand Pioneer Venus Multiprobe rather than just read about it. In short: The Pioneer Venus Multiprobe, also known as Pioneer Venus 2 or Pioneer 13, was a spacecraft launched in 1978 to explore Venus as part of NASA's Pioneer program. This part of the program included a spacecraft bus which was launched from Earth.

Pioneer Venus Multiprobe — main illustration
Pioneer Venus Multiprobe — illustration

Key takeaways

  • Pioneer Venus Multiprobe belongs to science; place it in that map before memorising details.
  • Learn the definition first, then one example that makes the definition concrete.
  • Connect Pioneer Venus Multiprobe to a quantity you can measure, compute or draw — that is where exam questions come from.
  • Reproduce the core statement of Pioneer Venus Multiprobe from memory before moving on to harder problems.

Reference excerpt

The Pioneer Venus Multiprobe, also known as Pioneer Venus 2 or Pioneer 13, was a spacecraft launched in 1978 to explore Venus as part of NASA's Pioneer program. This part of the program included a spacecraft bus which was launched from Earth. The bus carried one large and three smaller probes, which, after separating, each penetrated the Venusian atmosphere at a different location, returning data as they descended into the planet's thick atmosphere. The entries occurred on December 9, 1978.

In context There was also an orbiter launched in 1978, part of the overall Pioneer Venus project along with this entry probe mission. Whereas the probes entered the atmosphere in 1978, the Pioneer Venus Orbiter would stay in orbit throughout the 1980s and the early 1990s. The next major mission was the Magellan spacecraft, which was an orbiter capable of mapping Venus by seeing through its opaque clouds with radar.

Spacecraft

The Pioneer Venus Multiprobe bus was constructed by the Hughes Aircraft Company, built around the HS-507 bus. It was cylindrical in shape, with a diameter of 2.5 meters (8 ft 2 in) and a mass of 290 kilograms (640 lb). Unlike the probes, which did not begin making direct measurements until they had decelerated lower in the atmosphere, the bus returned data on Venus's upper atmosphere. The bus was targeted to enter the Venusian atmosphere at a shallow entry angle and transmit data until destruction by the heat of atmospheric friction. The objective was to study the structure and composition of the atmosphere down to the surface, the nature and composition of the clouds, the radiation field and energy exchange in the lower atmosphere, and local information on atmospheric circulation patterns. With no heat shield or parachute, the bus made upper atmospheric measurements with two instruments:

BIMS – an ion mass spectrometer to determine the origin and long-term development of the Venusian atmosphere, the dynamics of the upper atmosphere layers, its energy balance and the effect of solar radiation and interplanetary space on those layers. This instrument had a range of 1 to 46 u, used 6 W of power and weighed 5 kilograms (11 lb). BNMS – a neutral mass spectrometer. This made measurements of the interaction between the solar wind and Venus, the photochemistry of the upper layers of and heat distribution in the Venusian atmosphere. It had a range of 1 to 60 u, weighed 1 kilogram (2.2 lb), and used ~1 W of power. The spacecraft operated down to an altitude of about 110 kilometres (68 mi) before disintegrating.

Probes The spacecraft carried one large and three small atmospheric probes, designed by Senior Scientist and Program Manager Irwin Baker of Hughes Aircraft Company, to collect data as they descended into the atmosphere of Venus. The probes did not carry photographic instruments, and were not designed to survive landing—the smaller probes were not equipped with parachutes, and the larger probe's parachute was expected to detach as it neared the ground. All four probes continued transmitting data until impact; however, one survived and continued to transmit data from the surface, and another transmitted for 2 seconds after landing.

Large probe

The large probe carried seven experiments, contained within a sealed spherical pressure vessel. The science experiments were:

LNMS – neutral mass spectrometer to measure the atmospheric composition LGC – gas chromatograph to measure the atmospheric composition LSFR – solar flux radiometer to measure solar flux penetration in the atmosphere LIR – infrared radiometer to measure distribution of infrared radiation LCPS – cloud particle size spectrometer to measure particle size and shape LN – nephelometer to search for cloud particles temperature, pressure, and acceleration sensors This pressure vessel was encased in a nose cone and aft protective cover. After deceleration from initial atmospheric entry at about 11.5 kilometers per second (7.1 mi/s) near the equator on the night side of Venus, a parachute was deployed at 67 kilometres' (42 mi) altitude. The large probe was about 150 centimeters (59 in) in diameter and the pressure vessel itself was 73.2 centimeters (28.8 in) in diameter.

Small probes

Three identical small probes, around 0.8 meters (2 ft 7 in) in diameter, were deployed. These probes consisted of spherical pressure vessels surrounded by an aeroshell, but unlike the large probe, they had no parachutes and the aeroshells did not separate from the probes. The science experiments were:

a neutral mass spectrometer to measure the atmospheric composition a gas chromatograph to measure the atmospheric composition SNFR – solar flux radiometer to measure solar flux penetration in the atmosphere an infrared radiometer to measure distribution of infrared radiation MTUR – cloud particle size spectrometer to measure particle size and shape SN – nephelometer to search for cloud particles SAS – temperature, pressure, and acceleration sensors The radio signals from all four probes were also used to characterize the winds, turbulence, and propagation in the atmosphere. The small probes were each targeted at different parts of the planet and were named accordingly.

The North probe entered the atmosphere at about 60 degrees north latitude on the day side. The Night probe entered on the night side. The Day probe entered well into the day side, and was the only one of the four probes which continued to send radio signals back after impact, for over an hour.

Launch The Pioneer Venus Multiprobe was launched by an Atlas SLV-3D Centaur-D1AR rocket, which flew from Launch Complex 36A at the Cape Canaveral Air Force Station. The launch occurred at 07:33 on August 8, 1978, and deployed the Multiprobe into heliocentric orbit for its coast to Venus.

Arrival at Venus Prior to the Multiprobe reaching Venus, the four probes were deployed from the main bus. The large probe was released on November 16, 1978, and the three small probes on November 20. All four probes and the bus reached Venus on December 9, 1978. The large probe was the first to enter the atmosphere, at 18:45:32 UTC, followed over the next 11 minutes by the other three probes. The bus entered the atmosphere at 20:21:52 UTC and returned its last signal at 20:22:55 from an altitude of 110 kilometres (68 mi). The four probes transmitted data until they impacted the surface of Venus. The Day Probe survived the impact, returning data from the surface for 67 minutes and 37 seconds after reaching the surface.

… excerpt ends here. Continue reading the full article.

Illustrations

Pioneer Venus Multiprobe illustration
Pioneer Venus Multiprobe: Pioneer Venus Bus with probes attached
Pioneer Venus Bus with probes attached
Pioneer Venus Multiprobe: Pioneer Venus Large Probe opens its parachute (artist's rendition).
Pioneer Venus Large Probe opens its parachute (artist's rendition).
Pioneer Venus Multiprobe: A small probe (1-antenna, 2-temperature sensor, 3-frontal protection, 4-hermetic container, 5-nephelometer, 6-radiometer)
A small probe (1-antenna, 2-temperature sensor, 3-frontal protection, 4-hermetic container, 5-nephelometer, 6-radiometer)
Pioneer Venus Multiprobe: Entry of Pioneer Venus Multiprobe (comprising 1 large and 3 small probes)
Entry of Pioneer Venus Multiprobe (comprising 1 large and 3 small probes)

Worked examples

Example 1 — a first encounter with Pioneer Venus Multiprobe

Start with the simplest possible case. Write down what Pioneer Venus Multiprobe claims or describes in one sentence, then invent the smallest concrete situation in which that sentence is true. In science, the smallest case is usually a single object, a single equation or a single measurement. Check that every symbol or term in your sentence has a meaning in that case.

Example 2 — changing one variable

Take the situation from Example 1 and change exactly one quantity: double it, halve it, or set it to zero. Predict what should happen to Pioneer Venus Multiprobe before you calculate. Comparing your prediction with the result is the fastest way to find out whether you understand the idea or only the words.

Example 3 — an exam-style question

Typical questions about Pioneer Venus Multiprobe ask you to (a) state it precisely, (b) apply it to given data, and (c) explain a limitation. Practise writing all three answers in under five minutes; the third part is what separates a full-mark answer from an average one.

Applications of Pioneer Venus Multiprobe

In research
Pioneer Venus Multiprobe appears in science research whenever the underlying quantities have to be modelled precisely. Papers usually cite it as a starting assumption and then explore where it breaks down.
In technology and industry
Engineering practice reuses Pioneer Venus Multiprobe in design rules, simulations and safety margins. Knowing the idea lets you read a specification sheet and understand why the numbers look the way they do.
In the classroom
Pioneer Venus Multiprobe is common in secondary-school and first-year university syllabi. It links to neighbouring topics 1978 in spaceflight, Helen Planitia quadrangle, Ishtar Terra quadrangle, so understanding it makes those chapters shorter.
In everyday life
Look for Pioneer Venus Multiprobe outside the textbook — in sport, cooking, traffic, electronics or the sky above you. An example you found yourself is remembered far longer than one you were given.
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How to study Pioneer Venus Multiprobe in 20 minutes

  1. Read the reference excerpt below once, without taking notes.
  2. Close the page and write down what Pioneer Venus Multiprobe means in your own words.
  3. Compare your version with the excerpt and mark what you missed.
  4. Work through the three examples above with pen and paper.
  5. Explain Pioneer Venus Multiprobe out loud to somebody else — or to Teacher Smith in the lgStudy chat.

Frequently asked questions

What is Pioneer Venus Multiprobe in simple terms?

The Pioneer Venus Multiprobe, also known as Pioneer Venus 2 or Pioneer 13, was a spacecraft launched in 1978 to explore Venus as part of NASA's Pioneer program. This part of the program included a spacecraft bus which was launched from Earth.

Why does Pioneer Venus Multiprobe matter?

Because it connects several science ideas at once: it gives you a definition you can apply, a quantity you can calculate, and a way to check whether a result is plausible.

How should I study Pioneer Venus Multiprobe?

Read the excerpt, restate it from memory, then work through the examples and applications listed on this page. The five-step study plan above takes about twenty minutes.

What does this page cover?

It gives you a compact reference excerpt plus original lgStudy explanations, examples, applications and study material on Pioneer Venus Multiprobe.

Tags

  • 1978 in spaceflight
  • Helen Planitia quadrangle
  • Ishtar Terra quadrangle
  • Lavinia Planitia quadrangle
  • NASA missions to Venus
  • Pioneer program
  • Sedna Planitia quadrangle
  • Spacecraft launched in 1978
  • Venus aircraft
  • Venus landers

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