Venus Flashcards

1
Q

whats is the mass of venus compared to earth?

A

0.82 x

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2
Q

what is the radius of venus compares to earth?

A

0.95 x

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3
Q

what is the surface gravity of venus compared to earth?

A

0.9 x

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4
Q

what is the mean orbital radius?

A

0.72 au , almost circular

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5
Q

what is the maximum elongation of venus?

A

48 degrees from sun as seen from earth

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6
Q

what is the albedo?

A

76%, brightest object in sky after sun and moon

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7
Q

does venus have phases?

A

yes, bigger than mercurys’ and can be seen with binoculars.

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8
Q

what phase of venus is the brightest?

A

crescent

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9
Q

when is venus visible?

A

evening or morning.

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10
Q

rotation period of venus?

A

ranges from 22 hours up to 224.7 days

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11
Q

what did photographic observations show in 1950s?

A

a y shaped feature gave a 4 day retrograde (reverse) rotation.

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12
Q

what did radar measurements show in 1961?

A

surface rotated in a period of 243 days and was retrograde

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13
Q

why does venus have a high albedo?

A

clouds of venus reflect sunlight

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14
Q

what did spectroscopic measurements in 1930 show?

A

CO2 major constituent

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15
Q

what did radio observations show?

A

that surface temp is hot about 500 degrees

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16
Q

what is the composition of the atmosphere?

A
96% carbon dioxide
3.5% nitrogen
traces of so2 
water vapor h20
sulphuric acid h2s04 (acid rain)
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17
Q

what is the temp at the cloud tops?

A

-30 degrees

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18
Q

what is the pressure at the surface?

A

90 atmospheres

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19
Q

what distances do the sulfuric acid clouds form?

A

between 48-60 km from ground

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20
Q

how is the expected temperature calculated?

A

Tplanet = TSun (1 − a)^0.25√RSun/2d

Tplanet= expected temp in kelvin of planet
d= distance from sun
a= albedo (a=1 then 100% reflection)
21
Q

why is venus much hotter?

A

green house gases
visible light penetrates clouds and gets to surface- warmed and re-radiates in the infrared.
re-radiated energy is absorbed and heat is trapped near surface

22
Q

what did mariner 10?

A

flyby photos of cloud tops taken in ultraviolet showed rapidly moving circulation, only 4 days to circle planet speeds of 360 km/h- retrograde direction

23
Q

what did veneras do?

A

beneath clouds, landing probes on surface

24
Q

what did veneras find out?

A
hostile planet
90x pressure that earth at sea level
landscape- heap of stones- sharp edges and smooth
wind speeds sluggish
sunlight casts shadows
25
what did the pioneer venus orbiter do?
moniter cloud motions, while probes recorded data on temp, pressure and composition with altitude
26
what did the magellan do?
detailed radar map of entire surface- no magnetic field
27
what did venus express do and when launched?
nov 2005 arrived april 2006 found evidence for past oceans and confirmed presence of lightning by studying atmosphere and clouds
28
what did venera 9 show?
scree on a hill (15-25 degrees) slope, field of flat boulders,separated by sharp stones and dust
29
what did venera 10 show?
older more weathered, smoother surface | gamma ray spectrometer revealed volcanic rock, basalt
30
what did venera 13 show?
phoebe regio: rock-strewn plain, with outcrops and patches of dark, fine-grained material. evidence of chemical erosion. soil showed basalt and potassium
31
what did venera 14 show?
less-fine grained material regular layers of rocky,broken plates basalts similar to earths seabed
32
average density of venus?
5.3 g/cm^3
33
which features reflect better?
a hard flat surface better than powdered one | earth facing slope better than oblique
34
what was the pioneer venus the first to attempt 1978?
orbit radar around venus
35
how did the pioneer venus take its recordings?
using radar altimeter which bounced microwaves off surface. Built up a map in strips as venus rotated. mapped 93% of surface- resolution of 50km
36
what are the 3 general types of terrain on venus?
1: rolling plains (65%) 2: highlands (8%) 3: lowlands (27%)
37
Describe features of rolling plains
lying within 500m of mean level, numerous craters and circular basins, some filled with lava. Some volcanic, some impact large and shallow.
38
what are the three major regions of highlands?
ishtar terra, aphrodite terra, beta regio
39
what are the features of ishtar terra?
size of australia. lofty plateau (3km). several mountains, including maxwell montes which is highest of venus volcanic region
40
what are the features of aphrodite terra?
size of africa, rough and broken mountains
41
what are the features of beta regio?
two large shield volcanoes, rhea and theia mons. 4km high and lie on fault line.
42
what do the valley and trench systems imply?
tectonic activity played a role in formation of these regions
43
why does water vapour increase green house gases on venus compared to earth?
no seas to dissolve co2 it in.
44
what did eventually happen with the water?
dissociated into hydrogen which escapes and oxygen which reacted with rocks
45
what is a transit of mercury and venus?
because closer to sun, get between earth and sun on occasion and can be seen as dark discs moving across solar surface
46
why is there more opportunities to see a transit of mercury?
orbits the sun more quickly
47
why does the geometric alignment of mercury only occur every 7 years in may or november?
the plane of mercurys orbit is tilted by 7 degrees with respect to that of earth
48
what is the orbital plane of venus with respect to earths orbit?
inclined by 3.4 degrees so takes 8 years in pairs in june or december, each pair separated by 106 or 121 years
49
what can transits be used for?
to measure parallax angle