Cytherocentric orbit

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Animation of JAXA probe Akatsuki's trajectory around Venus from 1 December 2015

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Akatsuki *
Venus Animation of Akatsuki trajectory around Venus.gif
Animation of JAXA probe Akatsuki's trajectory around Venus from 1 December 2015
  Akatsuki ·   Venus

A Cytherocentric orbit is an orbit around the planet Venus. Venus has no moon, but several man-made objects orbit the planet.

Contents

The name is analogous to the term "geocentric orbit" for an orbit around Earth and "heliocentric orbit" for an orbit around the Sun. The apsides of an Cytherocentric orbit are pericytherion, the pericenter (analogous to "perigee"), and the apocenter is named apocytherion (analogous to "apogee").

Etymology

The Cythero prefix is derived from Kythira or "Cythera." In Greek mythology, Cythera was an island associated with the goddess Aphrodite, who is the equivalent of the Roman goddess Venus. Therefore, naming an orbit around Venus "cytherocentric" is a way of referencing Venus' association with this goddess.[ citation needed ]

Satellites in Cytherocentric orbit

Venera 9 was the first satellite to achieve Venus orbit in 20 October 1975. Akatsuki was the latest probe to achieve Venus orbit in 2015. [1]

Eight probes have achieved Venus orbit:

In order to enter Venus orbit, a satellite has to perform an engine burn to reduce the speed. Otherwise, the probe moves too fast to achieve orbit and will be a flyby. A noteworthy case is that of Japanese probe Akatsuki, which failed to enter orbit around Venus on 6 December 2010. [2] JAXA stated on 8 December that the probe's orbital insertion maneuver had failed, [3] because of a defect in the orbital insertion burn. After the craft orbited the Sun for five years, engineers successfully placed it into an alternative Venusian elliptic orbit on 7 December 2015 by firing its attitude control thrusters for 20 minutes.

Magellan was the first interplanetary probe to use aerobraking to reduce the apocytherion. [4] By passing through the dense atmosphere, a probe can reduce its speed and attain the necessary delta-v. Venus's thick atmosphere supports aerobraking. This reduces fuel needs.

Stationary and synchronous orbits

A satellite with revolutionary period that matches the planet's rotational period appears fixed at a position in the sky relative to an observer on the planet. Such an orbit on Earth is a Geostationary orbit. [5]

The height of a stationary or synchronous orbit can be calculated as follows:

[6]

where G is the gravitational constant , m2 is the mass of the celestial body, and T is the sidereal rotational period of the body.

By this formula one can find the geostationary-analogous cytherostationary orbit. Around Venus, such an orbit would be 1,536,600 km or about 253 Venus radii from the planet's surface. This is because Venus has the slowest rotation rate of any planet. The slower the rotation, the farther away a satellite must be in order to be stationary. The hill sphere of a celestial body describes the region in which the gravity of that body is dominant. The hill sphere radius of Venus is about 1 million kilometers; and as the cytherostationary orbital distance lies outside of it, no stable cytherostationary satellite can exist.

See also

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<span class="mw-page-title-main">Venus</span> Second planet from the Sun

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<span class="mw-page-title-main">Venera</span> Soviet program that explored Venus with multiple probes

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<span class="mw-page-title-main">Aerobraking</span> Spaceflight maneuver

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<i>Magellan</i> (spacecraft) NASA mission to map the surface of Venus via robotic probe (launched 1989)

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<span class="mw-page-title-main">JAXA</span> Japans national air and space agency

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<i>Akatsuki</i> (spacecraft) JAXA mission to study Venus via orbiting probe (2010–present)

Akatsuki, also known as the Venus Climate Orbiter (VCO) and Planet-C, is a Japan Aerospace Exploration Agency (JAXA) space probe tasked with studying the atmosphere of Venus. It was launched aboard an H-IIA 202 rocket on 20 May 2010, but failed to enter orbit around Venus on 6 December 2010. After the craft orbited the Sun for five years, engineers successfully placed it into an alternative Venusian elliptic orbit on 7 December 2015 by firing its attitude control thrusters for 20 minutes and made it the first Japanese satellite orbiting Venus.

Orbit insertion is the spaceflight operation of adjusting a spacecraft’s momentum, in particular to allow for entry into a stable orbit around a planet, moon, or other celestial body. This maneuver involves either deceleration from a speed in excess of the respective body’s escape velocity, or acceleration to it from a lower speed.

<span class="mw-page-title-main">Aphrodite Terra</span> Highland region on Venus, near the equator

Aphrodite Terra is one of the three continental regions on the planet Venus, the others being Ishtar Terra and Lada Terra. It is named for Aphrodite, the Greek equivalent of the goddess Venus, and is found near the equator of the planet. Aphrodite Terra is about half the size of Africa, making it the largest of the terrae.

<span class="mw-page-title-main">Observations and explorations of Venus</span>

Observations of the planet Venus include those in antiquity, telescopic observations, and from visiting spacecraft. Spacecraft have performed various flybys, orbits, and landings on Venus, including balloon probes that floated in the atmosphere of Venus. Study of the planet is aided by its relatively close proximity to the Earth, compared to other planets, but the surface of Venus is obscured by an atmosphere opaque to visible light.

<span class="mw-page-title-main">Atmosphere of Venus</span> Gas layer surrounding Venus

The atmosphere of Venus is primarily of supercritical carbon dioxide and is much denser and hotter than that of Earth. The temperature at the surface is 740 K, and the pressure is 93 bar (1,350 psi), roughly the pressure found 900 m (3,000 ft) underwater on Earth. The Venusian atmosphere supports opaque clouds of sulfuric acid, making optical Earth-based and orbital observation of the surface impossible. Information about the topography has been obtained exclusively by radar imaging. Aside from carbon dioxide, the other main component is nitrogen. Other chemical compounds are present only in trace amounts.

<span class="mw-page-title-main">Exploration of Mercury</span>

The exploration of Mercury has a minor role in the space interests of the world. It is the least explored inner planet. As of 2015, the Mariner 10 and MESSENGER missions have been the only missions that have made close observations of Mercury. MESSENGER made three flybys before entering orbit around Mercury. A third mission to Mercury, BepiColombo, a joint mission between the Japan Aerospace Exploration Agency (JAXA) and the European Space Agency, is to include two probes. MESSENGER and BepiColombo are intended to gather complementary data to help scientists understand many of the mysteries discovered by Mariner 10's flybys.

<span class="mw-page-title-main">Venus Orbiting Imaging Radar</span> Cancelled 1983 U.S. mission to Venus

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The following outline is provided as an overview of and topical guide to Venus:

References

  1. "Exploration: Venus". The National Aeronautics and Space Administration. 2010.
  2. JAXA's press briefing, 22:00, 7 December 2010 JST
  3. "Japan's Venus Probe Fails to Enter Orbit". ABC News . Retrieved 8 December 2010.
  4. Lyons, Daniel T.; Saunders, R. Stephen; Griffith, Douglas G. (1 May 1995). "The Magellan Venus mapping mission: Aerobraking operations". Acta Astronautica. 35 (9): 669–676. Bibcode:1995AcAau..35..669L. doi:10.1016/0094-5765(95)00032-U. ISSN   0094-5765.
  5. "Space Today Online - Answers To Your Questions". Spacetoday.org. 2010.
  6. "Calculating the Radius of a Geostationary Orbit - Ask Will Online". Ask Will Online. 2012-12-27. Retrieved 2017-11-21.