在希腊的时候有次和D开车去一个小海滩，车停海岸坡上，返回的时候我先走回岸上等他把车开过来，正好站在一幢大别墅院子旁边，里面养了一只大白熊犬。那只狗真的好大，高度差不多到我肚子，把嘴从铁门栏杆缝隙伸出来朝我吐舌头摇尾巴，我撸狗心切，试探着摸了一下确认狗子纯粹是想亲近我之后就开始沉浸式撸狗头，但那种体型的大狗其实最适合用力抱个满怀。
我观察了一下，偌大的院子里像是没有人，狗子也没给拴上，毛是修剪过的但是比较粗糙也有点脏，再加上见到陌生人就这么饥渴求撸，我怀疑是不是主人不常在家（那块海滩周围本来就没什么人）。等D把车开过来，我收手的时候狗子还恋恋不舍的看我，发出呜呜的声音。
甚至我上车离开的时候狗子还在院子里跑着追了我们一截，最后看着我们越走越远还叫了几声，现在想起来也觉得心软。
我跟D说dogs love humans better than humans do，他表示同意。
D在路上也经常喜欢逗别人院子里的狗，有次遇到大型看门狗，一边很凶地对我们叫，一边又摇着尾巴想接近，D就哈哈笑说他 really enjoys when guardian dogs are confused by their conflicting instincts to protect the house against strangers and the desire for some cuddling，也是够恶趣味的。
我观察了一下，偌大的院子里像是没有人，狗子也没给拴上，毛是修剪过的但是比较粗糙也有点脏，再加上见到陌生人就这么饥渴求撸，我怀疑是不是主人不常在家（那块海滩周围本来就没什么人）。等D把车开过来，我收手的时候狗子还恋恋不舍的看我，发出呜呜的声音。
甚至我上车离开的时候狗子还在院子里跑着追了我们一截，最后看着我们越走越远还叫了几声，现在想起来也觉得心软。
我跟D说dogs love humans better than humans do，他表示同意。
D在路上也经常喜欢逗别人院子里的狗，有次遇到大型看门狗，一边很凶地对我们叫，一边又摇着尾巴想接近，D就哈哈笑说他 really enjoys when guardian dogs are confused by their conflicting instincts to protect the house against strangers and the desire for some cuddling，也是够恶趣味的。
It's you again ?
" Hey y'all already know "
I need to invest my money into your entertainment company from now on ?
" Fxxk " My Money Men !!! [苦涩][汗][费解]
I thought I Ran as fast as I could , Cause Mr. Wang's Acting and singing Skills is bad as hell
but by the end of the day is you again !
" But Okay fine whatever "
2023 [打call]
" Hey y'all already know "
I need to invest my money into your entertainment company from now on ?
" Fxxk " My Money Men !!! [苦涩][汗][费解]
I thought I Ran as fast as I could , Cause Mr. Wang's Acting and singing Skills is bad as hell
but by the end of the day is you again !
" But Okay fine whatever "
2023 [打call]
Credits
ILLUSTRATION: NASA, ESA, Leah Hustak (STScI)
Scientists often classify spectra based on the key light–matter interactions they represent and how they are used.
Continuous Spectrum: A continuous spectrum contains all wavelengths of light in a certain range. Hot, dense light sources like stars, for example, emit a nearly continuous spectrum of light, which travels out in all directions and interacts with other materials in space. The broad range of colors that a star emits depends on its temperature.
Absorption Spectrum: When starlight passes through a cloud of gas, some of the light is absorbed and some is transmitted through the gas. TThe wavelengths of light that are absorbed depends on what elements and compounds it is made of. An absorption spectrum has dark lines or gaps in the spectrum corresponding to wavelengths that are absorbed by the gas.
Emission Spectrum: Starlight can also heat up a cloud of gas, exciting the atoms and molecules within the gas, and causing it to emit light. The spectrum of light that a cloud of gas emits depends on its temperature, density, and composition. An emission spectrum consists of a series of colored lines that correspond to wavelengths emitted by the glowing gas.
ILLUSTRATION: NASA, ESA, Leah Hustak (STScI)
Scientists often classify spectra based on the key light–matter interactions they represent and how they are used.
Continuous Spectrum: A continuous spectrum contains all wavelengths of light in a certain range. Hot, dense light sources like stars, for example, emit a nearly continuous spectrum of light, which travels out in all directions and interacts with other materials in space. The broad range of colors that a star emits depends on its temperature.
Absorption Spectrum: When starlight passes through a cloud of gas, some of the light is absorbed and some is transmitted through the gas. TThe wavelengths of light that are absorbed depends on what elements and compounds it is made of. An absorption spectrum has dark lines or gaps in the spectrum corresponding to wavelengths that are absorbed by the gas.
Emission Spectrum: Starlight can also heat up a cloud of gas, exciting the atoms and molecules within the gas, and causing it to emit light. The spectrum of light that a cloud of gas emits depends on its temperature, density, and composition. An emission spectrum consists of a series of colored lines that correspond to wavelengths emitted by the glowing gas.
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