The Chronicles of Local Space

A fictional exploration of nearby star systems

61 Virginis

Rava Ferrugo Formosis Humus Bellum Levitas Magnus Caeruleus Ovatus Nanus
A photomontage of the ten planets in the 61 Virginis system. The scale is one pixel per 300 kilometres.
The ten planets in the 61 Virginis system.
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The 61 Virginis System
Right Ascension 13h 18m
Declination −18° 19'
Distance 27.79 ± 0.16 ly
Spectral Class G5V
Estimated Mass 0.96 × Sol
Luminosity 0.78 × Sol

Star charts
61 Virginis
as seen from Sol.
Sol as seen from
61 Virginis.
61 Virginis as seen from Sol Sol as seen from 61 Virginis
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Brightest stars as seen from 61 Virginis
Includes all stars of magnitude 1.00 and brighter
Star Magnitude Distance
Arcturus −1.01 23.6
Canopus −0.63 307.2
Rigel 0.21 875.5
Beta Centauri (Hadar) 0.50 372.1
Betelgeuse 0.50 509.1
Achernar 0.59 148.8
Alpha Crucis (Acrux) 0.64 303.1
Spica 0.73 222.1
Theta Centauri (Menkent) 0.88 34.3
Alpha Aurigae (Capella) 0.91 62.8
Vega 0.97 38.7
Antares 0.99 534.3

61 Virginis is a sunlike star with a spectral type of G5V. It is located 27.79 light years from Sol. This star is slightly less massive than Sol, and has a lumosity of 0.78 Sols.

Local Space

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Stargates in this system
Destination Distance
Gliese 432 14.9
Gliese 581 14.4
Wolf 424 A 17.0

Probes from the Dandelion Project explored the system for the first time in 2930. The system has ten planets.

61 Virginis

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The planets of the 61 Virginis system
Planet SMA
(AU)
Orbital
Period
e Equatorial
Diameter
(km)
Mass
(Earths)
Density
(g/cm3)
Gravity
(Earth g)
Atmospheric
Pressure
(Earth=1)
Sidereal
Day
Mean
Solar
Day
Axial
Tilt
Known
Moons
Rava 0.2297 41.040 d 0.0038 4296 0.02723 3.92 0.2399 0.00000300 41d 00h 56.9m Synchronous 00° 03.7' 0
Ferrugo 0.3670 82.874 d 0.0092 7524 0.1778 4.76 0.5106 0.00653 82d 20h 58.6m Synchronous 01° 03.7' 0
Formosis 0.5942 170.75 d 0.0158 11300 0.6348 5.02 0.8088 34.2 14d 11h 29.4m 15d 19h 41.0m 03° 28.8' 0
Humus 1.011 1.0379 y 0.0144 14470 1.487 5.62 1.155 2.96 22h 25.5m 22h 28.8m 15° 07.3' 2
Bellum 1.609 2.0831 y 0.0722 11780 0.5779 4.04 0.6775 0.0757 1d 15h 35.6m R 1d 15h 30.5m 162° 38.3' 3
Levitas 6.229 15.865 y 0.1023 68970 31.28 1.18 1.069 &mdash 10h 32.5m R 10h 32.5m 102° 09.1' 14
Magnus 11.46 39.575 y 0.0055 123000 200.7 1.27 2.157 &mdash 14h 50.4m 14h 50.4m 13° 25.1' 14
Caeruleus 18.50 81.218 y 0.0129 68280 31.05 1.12 1.083 &mdash 17h 53.2m 17h 53.2m 06° 41.0' 15
Ovatus 27.47 146.91 y 0.0230 55810 16.35 1.26 0.8535 &mdash 07h 00.6m 07h 00.6m 28° 54.2' 11
Nanus 50.58 367.13 y 0.1266 30090 4.904 2.11 0.8809 &mdash 14h 50.7m 14h 50.7m 41° 30.6' 6
[ Skip Table ]
Natural satellites of the 61 Virginis system
Name Diameter
(km)
Period
(days)
Semimajor
Axis (km)
Ecc Inc
Natural Satellites of Humus
Orbis 1024 5.595 152000 0.0012 0.19
Lapis 53 17.12 320200 0.1574 5.42
Natural Satellites of Bellum
Pestis 39 2.144 58500 0.0135 1.49
Mors 77 5.040 103400 0.0265 2.00
Fames 25 14.60 210200 0.0362 158.19
Natural Satellites of Levitas
Levitas V 144 0.4803 81640 0.0002 0.00
Levitas VI 485 0.7741 112200 0.0159 0.02
Levitas I 1255 1.194 149800 0.0045 0.19
Levitas II 2030 2.996 276600 0.0082 0.17
Levitas III 1320 5.955 437300 0.0125 0.43
Levitas IV 1500 11.91 694400 0.0171 0.28
Levitas VII 623 29.64 1275000 0.0180 0.53
Levitas IX 115 29.64 1275000 0.0124 0.76
Levitas VIII 407 49.68 1799000 0.0220 4.53
Levitas X 91 89.96 2672000 0.2071 11.79
Levitas XI 38 285.4 5769000 0.1167 165.13
Levitas XII 50 388.3 7084000 0.2702 39.41
Levitas XIII 19 581.1 9269000 0.1462 147.69
Levitas XIV 31 581.3 9271000 0.1503 146.85
Natural Satellites of Magnus
Magnus V 126 0.8155 215900 0.0005 0.02
Magnus VI 329 1.222 282700 0.0015 0.04
Magnus IX 95 2.059 400200 0.0020 0.03
Magnus I 2103 3.094 525100 0.0026 0.08
Magnus II 3572 6.119 827400 0.0035 0.22
Magnus III 1470 12.26 1315000 0.0047 1.44
Magnus IV 943 24.72 2099000 0.0022 2.33
Magnus VII 325 36.65 2729000 0.0102 1.40
Magnus VIII 332 64.75 3988000 0.0785 3.65
Magnus XII 19 112.1 5749000 0.2775 158.27
Magnus X 16 199.9 8455000 0.3259 41.39
Magnus XI 23 218.2 8964000 0.3200 40.96
Magnus XIII 18 227.2 9208000 0.3112 149.69
Magnus XIV 16 308.0 11280000 0.4002 13.27
Natural Satellites of Caeruleus
Caeruleus VII 68 0.6762 102300 0.0010 0.00
Caeruleus VIII 60 0.7186 106500 0.0013 0.02
Caeruleus IX 52 0.7825 112700 0.0009 0.05
Caeruleus I 725 1.196 149600 0.0037 0.40
Caeruleus II 608 2.152 221300 0.0052 0.10
Caeruleus III 1340 3.581 310800 0.0044 0.24
Caeruleus IV 2038 5.380 407700 0.0016 0.38
Caeruleus V 1930 10.76 647000 0.0025 0.33
Caeruleus VI 907 26.84 1190000 0.0063 1.06
Caeruleus X 164 136.0 3512000 0.0466 7.73
Caeruleus XI 66 293.7 5867000 0.0682 19.73
Caeruleus XIV 41 312.5 6115000 0.0754 41.49
Caeruleus XII 71 451.5 7814000 0.1701 17.60
Caeruleus XIII 89 452.1 7822000 0.1693 17.55
Caeruleus XV 55 484.8 8194000 0.3683 155.78
Natural Satellites of Ovatus
Ovatus I 434 0.4333 61390 0.0001 0.00
Ovatus II 841 0.7236 86410 0.0008 0.01
Ovatus III 761 1.448 137200 0.0002 0.01
Ovatus IV 581 2.173 179900 0.0003 0.00
Ovatus V 450 3.612 252400 0.0014 0.01
Ovatus VI 211 31.22 1063000 0.0631 9.93
Ovatus VII 168 56.24 1574000 0.0496 2.50
Ovatus VIII 173 83.89 2055000 0.1236 26.10
Ovatus IX 82 104.3 2376000 0.1453 156.84
Ovatus X 64 161.1 3174000 0.1645 167.22
Ovatus XI 42 737.2 8749000 0.4413 32.16
Satellites of Ovatus XI
1 Ovatus XIA160.612467.660.0133 0.01
Natural Satellites of Nanus
Nanus III 481 0.7291 58140 0.0011 0.01
Nanus I 1832 1.093 76140 0.0040 0.04
Nanus II 1406 2.183 120800 0.0064 0.06
Nanus IV 788 5.473 222900 0.0134 0.06
Nanus V 198 22.61 573800 0.0362 1.16
Nanus VI 68 137.4 1912000 0.4160 29.44

Rava

Derivation of name: Latin for “gray” with feminine suffix

Rava is a small world with no appreciable atmosphere or geological activity. It is heavily cratered.

Ferrugo

Ferrugo

Derivation of name: Latin for “rust”

Ferrugo is a small, hot world with a thin atmosphere and covered with reddish dust. It is locked in synchronous rotation to its star. The synchronous rotation and thin atmosphere cause the less volatile gases such as water vapor and carbon dioxide to condense on the night side of the planet in a large ice cap. What atmosphere the planet still possesses is enriched with gases with lower condensation temperatures such as argon and nitrogen. The world has some craters, and the older craters show evidence of weathering by wind-borne dust.

Formosis

Formosis with Canopus.
Formosis with Canopus

Derivation of name: Latin for “beautiful”, an allusion to Venus

Formosis is a world resembling Venus. It has a thick, hot atmosphere composed primarily of carbon dioxide. Like many such worlds, Formosis has endured a runaway greenhouse effect. Its slow rotation is a consequence of tidal locking; although the tidal locking process is not yet complete it is far advanced.

Humus

Orbis at dusk on three consecutive evenings.
Orbis transits 61 Virginis in an annular solar eclipse.
Annular solar eclipse as seen from Humus

Derivation of name: Latin for “ground” or “soil”, an allusion to Earth

Out of all the systems explored within ten parsecs of the Sun, the world of Humus is the most Earthlike world discovered and explored so far. Humus is somewhat larger and more massive than the Earth, and this gives it a greater surface gravity. Its day is about seven per cent shorter than that of the Earth. The world is an active world — it has plate tectonics, rugged mountain ranges, and active volcanoes.

Humus has a thick atmosphere about three times as dense as the Earth’s atmosphere. Like Earth, the atmosphere is mainly composed of nitrogen (86.54%), oxygen (12.41%) and argon (0.83%), with carbon dioxide (0.22%) being more abundant than on Earth. Despite the relatively high atmospheric pressure, the atmosphere is breathable for humans because the partial pressures of the important atmospheric gases are all within the breathable ranges for humans.[1] The important gases are nitrogen (83% of maximum pressure for humans), oxygen (70% of maximum) and carbon dioxide (71% of maximum). On Humus, water boils at about 133.5°C.

Orbis and Lapis, showing the great difference in apparent size of these moons.
Orbis and Lapis

Humus has two moons. The larger moon, Orbis, orbits Humus in about five and a half days. Orbis is large enough to present familiar phases in the sky. Orbis cycles through its phases with disconcerting speed for an observer used to the leisurely cycle of phases of Earth’s moon: one night Orbis may be a thin crescent, on the next it has waxed to a half moon, and on the third it may be almost full. Even in the course of a single night, the phase of Orbis can change noticeably. Eclipse seasons for Orbis arrive around the time of the equinoxes. At these times, Orbis causes a series of three or four annular solar eclipses and experiences three or four total lunar eclipses. When Orbis eclipses the sun, the eclipse takes about fifteen minutes from start to finish.

The smaller moon of Lapis takes about 17 days to orbit once, and appears starlike due to its small size. Lapis is a moon with an irregular shape and is believed to be a captured planetoid.

Humus is home to alien life.

Bellum

Bellum

Derivation of name: Latin for “war”, an allusion to Mars

Bellum is an ice-covered world that resembles Europa, except it is much larger and the ice is smoother. The smoothness of the ice suggests that the world has a liquid ocean under the surface ice.

Superficially, Bellum strongly resembles its sibling world of Formosis; both worlds are of a similar size and from space appear as bright white orbs. The two world are quite different, however. Formosis is hot and dry and its appearance are due to thick clouds in a thick atmosphere, whereas Bellum is an ice-covered world with a thin atmosphere.

Bellum has a retrograde rotation. It also has three moons in direct orbits from the planet’s perspective. The moons and retrograde rotation are believed to originate from a planetary collision early in the history of this star system. For this reason, Bellum and its three moons are named after the Four Horsemen of the Apocalypse.

Levitas

Levitas as seen from Humus

Derivation of name: Latin for “lightness” because the planet is of relatively low mass

Levitas is an odd world. In general appearance it is a small gas giant with about one third the mass of Saturn. The most striking feature of Levitas is the planet’s 102-degree axial tilt. This tilt is similar to Uranus in the Sol system, and is believed to have originated in a similar way — a planetary collision during the formation of the 61 Virginis system.

Levitas has a wide but fairly faint ring system. The world has 14 known moons, the four largest of which have diameters greater than 1000 kilometres.

Magnus

Magnus

Derivation of name: Latin for “large”

The gas giant Magnus is the most massive planet in the 61 Virginis system. Its mass is about 0.63 Jupiter masses, and it orbits 61 Virginis with a period of about 39.5 Julian years.

Caeruleus

Caeruleus

Derivation of name: Latin for “dark blue”

Caeruleus is a large Neptune-class planet that resembles Neptune in appearance.

Ovatus

Ovatus

Derivation of name: Latin for “oval”

Ovatus is another Neptunelike world. Its rotation is unusually fast — one rotation takes just seven hours. This very rapid rotation gives the world a noticeably oblate shape, from which the world gets its name.

The moon Ovatus XI has its own satellite, Ovatus XIA. Satellite moons are unusual because most satellites are tidally locked to their planets which makes it impossible for satellite moons to have stable orbits. Ovatus XI lies outside the tidal lock radius of Ovatus which permits Ovatus XI to have its own moon.

Nanus

Nanus

Derivation of name: Latin for “dwarf”

Nanus is an unusual world. It is an ice subgiant, which is a world like an ice giant but smaller in size. Nanus has a mass only about five times that of the Earth.


Further reading

References

  1. Stephen H. Dole, Habitable Planets for Man, Blaisdell Publishing Company, New York USA, 1964, pp. 15–16.

Nonfictional links

Just the facts.

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